# pdgfootnote

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AABOUD 2019AT searched in 36.1 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for metastable and stable R-hadrons. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined. No significant deviations from the expected Standard Model background are observed. Gluino R-hadrons with lifetimes of the order of 50 ns are excluded at 95% C.L. for masses below 1980 GeV using the muon-spectrometer agnostic analysis. Using the full-detector search, the observed lower limits on the mass are 2000 GeV. See their Figure 9 (top).


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AABOUD 2019C searched in 36.1 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for metastable and stable R-hadrons arising as excesses in the mass distribution of reconstructed tracks with high transverse momentum and large dE/dx. Gluino R-hadrons with lifetimes above 10 ns are excluded at 95% C.L. with lower mass limit range between 1000 GeV and 2060 GeV, see their Figure 5(a). Masses smaller than 1290 GeV are excluded for a lifetime of 1 ns, see their Figure 6. In the case of stable R-hadrons, the lower mass limit is 1890 GeV, see their Figure 5(b).


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SIRUNYAN 2019BT searched in 137 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for long-lived particles decaying to displaced, nonprompt jets and missing transverse momentum.  Candidate signal events are identified using the timing capabilities of the CMS electromagnetic calorimeter. The results of the search are found to be consistent with the background predictions. Limits are set on the gluino mass in a GMSB model where long-lived gluinos are pair produced and decaying via gtilde --> g Gtilde, see their Figures 4 and 5.


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AABOUD 2018S searched in 32.8 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for long-lived gluinos in final states with large missing transverse momentum and at least one high-mass displaced vertex with five or more tracks. The observed yield is consistent with the expected background. Exclusion limits are derived for Tglu1A models predicting the existence of long-lived gluinos reaching roughly m(gtilde) = 2000 GeV to 2370 GeV for m(chitilde_{{1}}()0) = 100 GeV and gluino lifetimes between 0.02 and 10 ns, see their Fig. 8. Limits are presented also as a function of the lifetime (for a fixed gluino-neutralino mass difference of 100 GeV) and of the gluino and neutralino masses (for a fixed lifetime of 1 ns). See their Fig. 9 and 10 respectively.


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KHACHATRYAN 2017AR searched in 17.6 fb^{-1} of p p collisions at sqrt(s) = 8 TeV for R-parity-violating SUSY in which long-lived neutralinos or gluinos decay into multijet final states. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass for a range of mean proper decay lengths (ctau), see their Fig. 7. The upper limits on the production cross section times branching ratio squared (Fig. 7) are also applicable to long-lived neutralinos.


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AABOUD 2016B searched in 3.2 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for long-lived R-hadrons using observables related to large ionization losses and slow propagation velocities, which are signatures of heavy charged particles traveling significantly slower than the speed of light. Exclusion limits at 95% C.L. are set on the long-lived gluino masses exceeding 1580 GeV. See their Fig. 5.


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AABOUD 2016C searched in 3.2 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for long-lived and stable R-hadrons identified by anomalous specific ionization energy loss in the ATLAS Pixel detector. Gluino R-hadrons with lifetimes above 0.4 ns are excluded at 95% C.L. with lower mass limit range between 740 GeV and 1590 GeV. In the case of stable R-hadrons, the lower mass limit is 1570 GeV. See their Figs. 5 and 6.


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KHACHATRYAN 2016BW searched in 2.5 fb^{-1} of p p collisions at sqrt(s) = 13 TeV for events with heavy stable charged particles, identified by their anomalously high energy deposits in the silicon tracker and/or long time-of-flight measurements by the muon system. No evidence for an excess over the expected background is observed. Limits are derived for pair production of gluinos as a function of mass, depending on the interaction model and on the fraction f, of produced gluinos hadronizing into a gtilde - gluon state, see Fig. 4 and Table 7.


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AAD 2015AE searched in 19.1 fb^{-1} of p p collisions at sqrt(s) = 8 TeV for heavy long-lived charged particles, measured through their specific ionization energy loss in the ATLAS pixel detector or their time-of-flight in the ALTAS muon system. In the absence of an excess of events above the expected backgrounds, limits are set R-hadrons in various scenarios, see Fig. 11. Limits are also set in LeptoSUSY models where the gluino decays to stable 300 GeV leptons, see Fig. 9.


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AAD 2015BM searched in 18.4 fb^{-1} of p p collisions at sqrt(s) = 8 TeV for stable and metastable non-relativistic charged particles through their anomalous specific ionization energy loss in the ATLAS pixel detector. In absence of an excess of events above the expected backgrounds, limits are set within a generic R-hadron model, on stable gluino R-hadrons (see Table 5) and on metastable gluino R-hadrons decaying to (g / q qbar) plus a light chitilde_{{1}}^0() (see Fig. 7) and decaying to t tbar plus a light chitilde_{{1}}()0 (see Fig. 9).


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KHACHATRYAN 2015AK looked in a data set corresponding to 18.6 fb**-1 of p p collisions at sqrt(s) = 8 TeV, and a search interval corresponding to 281 h of trigger lifetime, for long-lived particles that have stopped in the CMS detector. No evidence for an excess over the expected background in a cloud interaction model is observed. Assuming the decay gtilde --> g chitilde_1()0 and lifetimes between 1 mus and 1000 s, limits are derived on gtilde production as a function of mass(chitilde_{{1}}()0), see Figs. 4 and 6. The exclusions require that mass(chitilde_{{1}}()0) is kinematically consistent with the minimum values of the jet energy thresholds used.


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AAD 2013AA searched in 4.7 fb**-1 of p p collisions at sqrt(s) = 7 TeV for events containing colored long-lived particles that hadronize forming R-hadrons. No significant excess above the expected background was found. Long-lived R-hadrons containing a gtilde are excluded for masses up to 985 GeV at 95% C.L in a general interaction model. Also, limits independent of the fraction of R-hadrons that arrive charged in the muon system were derived, see Fig. 6.


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AAD 2013BC searched in 5.0 fb**-1 of p p collisions at sqrt(s) = 7 TeV and in 22.9 fb**-1 of p p collisions at sqrt(s) = 8 TeV for bottom squark R-hadrons that have come to rest within the ATLAS calorimeter and decay at some later time to hadronic jets and a neutralino. In absence of an excess of events above the expected backgrounds, limits are set on gluino masses for different decays, lifetimes, and neutralino masses, see their Table 6 and Fig. 10.


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CHATRCHYAN 2013AB looked in 5.0 fb**-1 of p p collisions at sqrt(s) = 7 TeV and in 18.8 fb**-1 of p p collisions at sqrt(s) = 8 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of gtilde's. No evidence for an excess over the expected background is observed. Limits are derived for pair production of gluinos as a function of mass (see Fig. 8 and Table 5), depending on the fraction, f, of formation of gtilde-g (R-gluonball) states. The quoted limit is for f = 0.1, while for f = 0.5 it degrades to 1276 GeV. In the conservative scenario where every hadronic interaction causes it to become neutral, the limit decreases to 928 GeV for f = 0.1.


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AAD 2012P looked in 31 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with pair production of long-lived gluinos. The hadronization of the gluinos leads to R-hadrons which may stop inside the detector and later decay via gtilde --> g chitilde_1()0 during gaps between the proton bunches. No significant excess over the expected background is observed. From a counting experiment, a limit at 95% C.L. on the cross section as a function of mass(gtilde) is derived for mass(chitilde_{{1}}()0) = 100 GeV, see Fig. 4. The limit is valid for lifetimes between E-5 and E3 seconds and assumes the Generic matter interaction model for the production cross section.


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CHATRCHYAN 2012AN looked in 4.0 fb**-1 of p p collisions at sqrt(s) = 7 TeV for events with pair production of long-lived gluinos. The hadronization of the gluinos leads to R-hadrons which may stop inside the detector and later decay via gtilde --> g chitilde_1()0 during gaps between the proton bunches. No significant excess over the expected background is observed. From a counting experiment, a limit at 95% C.L. on the cross section as a function of mass(gtilde) is derived, see Fig. 3. The mass limit is valid for lifetimes between E-5 and E3 seconds, for what they call ''the daughter gluon energy E_{{g}}() >'' 100 GeV and assuming the cloud interaction model for R-hadrons. Supersedes KHACHATRYAN 2011.


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CHATRCHYAN 2012L looked in 5.0 fb**-1 of p p collisions at sqrt(s) = 7 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of gtilde's. No evidence for an excess over the expected background is observed. Limits are derived for pair production of gluinos as a function of mass (see Fig. 3), depending on the fraction, f, of formation of gtilde-g (R-glueball) states. The quoted limit is for f = 0.1, while for f = 0.5 it degrades to 1046 GeV. In the conservative scenario where every hadronic interaction causes it to become neutral, the limit decreases to 928 GeV for f=0.1. Supersedes KHACHATRYAN 2011C.


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AAD 2011K looked in 34 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or time of flight in the tile calorimeter, from pair production of gtilde. No evidence for an excess over the SM expectation is observed. Limits are derived for pair production of gluinos as a function of mass (see Fig. 4), for a fraction, f = 10%, of formation of gtilde-g (R-gluonball). If instead of a phase space driven approach for the hadronic scattering of the R-hadrons, a triple-Regge model or a bag-model is used, the limit degrades to 566 and 562 GeV, respectively.


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AAD 2011P looked in 37 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with heavy stable particles, reconstructed and identified by their time of flight in the Muon System. There is no requirement on their observation in the tracker to increase the sensitivity to cases where gluinos have a large fraction, f, of formation of neutral gtilde-g (R-gluonball). No evidence for an excess over the SM expectation is observed. Limits are derived as a function of mass (see Fig. 4), for f=0.1. For fractions f = 0.5 and 1.0 the limit degrades to 537 and 530 GeV, respectively.


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KHACHATRYAN 2011 looked in 10 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with pair production of long-lived gluinos. The hadronization of the gluinos leads to R-hadrons which may stop inside the detector and later decay via gtilde --> g chitilde_1^0() during gaps between the proton bunches. No significant excess over the expected background is observed. From a counting experiment, a limit at 95% C.L. on the cross section times branching ratio is derived for mass(gtilde)-mass(chitilde_{{1}}^0())> 100 GeV, see their Fig. 2. Assuming 100% branching ratio, lifetimes between 75 ns and 3E5 s are excluded for mass(gtilde) = 300 GeV. The gtilde mass exclusion is obtained with the same assumptions for lifetimes between 10 mu s and 1000 s, but shows some dependence on the model for R-hadron interactions with matter, illustrated in Fig. 3. From a time-profile analysis, the mass exclusion is 382 GeV for a lifetime of 10 mu s under the same assumptions as above.


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KHACHATRYAN 2011C looked in 3.1 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of gtilde. No evidence for an excess over the expected background is observed. Limits are derived for pair production of gluinos as a function of mass (see Fig. 3), depending on the fraction, f, of formation of gtilde-g (R-gluonball). The quoted limit is for f=0.1, while for f=0.5 it degrades to 357 GeV. In the conservative scenario where every hadronic interaction causes it to become neutral, the limit decreases to 311 GeV for f=0.1.


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AAD 2015BH searched in 20.3 fb^{-1} of p p collisions at sqrt(s) = 8 TeV for associated production of a light gravitino and a squark or gluino. The squark (gluino) is assumed to decay exclusively to a quark (gluon) and a gravitino. No evidence was found for an excess above the expected level of Standard Model background and 95% C.L. lower limits were set on the gravitino mass as a function of the squark/gluino mass, both in the case of degenerate and non-degenerate squark/gluino masses, see Figs. 14 and 15.


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ABDALLAH 2005B use data from sqrt(s) = 180 -- 208~GeV. They look for events with a single photon + notE final states from which a cross section limit of sigma < 0.18~pb at 208~GeV is obtained, allowing a limit on the mass to be set. Supersedes the results of ABREU 2000Z.


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ACHARD 2004E use data from sqrt(s) = 189 -- 209~GeV. They look for events with a single photon + notE final states from which a limit on the Gravitino mass is set corresponding to sqrt(F) > 238~GeV. Supersedes the results of ACCIARRI 1999R.


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ACOSTA 2002H looked in 87 pb**-1 of p pbar collisions at sqrt(s)=1.8 TeV for events with a high-E(T) photon and notET. They compared the data with a GMSB model where the final state could arise from q qbar --> Gtilde Gtilde gamma. Since the cross section for this process scales as 1/|F |**4, a limit at 95% CL is derived on |F |**1/2 > 221 GeV. A model independent limit for the above topology is also given in the paper.


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AAD 2024AH combined a number of ATLAS analyses to use them and interpret in a series of models derived from a flat-prior scan to pMSSM parameter space. Limits are provided in terms of fraction of models excluded as a function of one or two parameters, while marginalising over the others.


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AAD 2020C uses a statistical combination of six final states b bbar b bbar, b bbar W W, b bbar tau tau, W W W W, b bbar gamma gamma, and W W gamma gamma to search for non-resonant and resonant production of Higgs boson pairs. The search uses 36.1 fb^{-1} of p p collisions data at sqrt(s) = 13 TeV. Constraints in the habemus Minimal Supersymmetric Standard Model in the (mass(A), tanbeta) parameter space are placed, see their Figure 7(b).


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AAD 2020L used 27.8 fb^{-1} of p p collision data at sqrt(s) = 13 TeV to search for heavy neutral Higgs bosons produced in association with at least one b-quark and decaying into a pair of b-quarks. The data are compatible with SM expectations, yielding no significant excess of events in the mass range 450 -- 1400 GeV, see their Fig. 11. Exclusion limits at 95% C.L. were derived in hMSSM scenarios as a function of mass(A) and tanbeta, see their Fig. 9 and 10.


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AABOUD 2016AF uses a selection of searches by ATLAS for the electroweak production of SUSY particles studying resulting constraints on dark matter candidates. They use 20 fb**-1 of p p collisions at sqrt(s) = 8 TeV. A likelihood-driven scan of an effective model focusing on the gaugino-higgsino and Higgs sector of the pMSSM is performed. The ATLAS searches impact models where mass(chi_{{1}}()0) < 65 GeV, excluding 86% of them. See their Figs. 2, 4, and 6.


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AAD 2016AG searches for prompt lepton-jets using 20 fb**-1 of p p collisions at sqrt(s) = 8 TeV collected with the ATLAS detector. Lepton-jets are expected from decays of low-mass dark photons in SUSY-portal and Higgs-portal models. No significant excess of events is observed and 95% CL upper limits are computed on the production cross section times branching ratio for two prompt lepton-jets in models predicting 2 or 4 gamma_{{d}} via SUSY-portal topologies, for gamma_{{d}} mass values between 0 and 2 GeV. See their Figs 9 and 10. The results are also interpreted in terms of a 90% CL exclusion region in kinetic mixing and dark-photon mass parameter space. See their Fig. 13.


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AAD 2013P searched in 5 fb**-1 of p p collisions at sqrt(s) = 7 TeV for single lepton-jets with at least four muons; pairs of lepton-jets, each with two or more muons; and pairs of lepton-jets with two or more electrons. All of these could be signatures of Hidden Valley supersymmetric models. No statistically significant deviations from the Standard Model expectations are found. 95% C.L. limits are placed on the production cross section times branching ratio of dark photons for several parameter sets of a Hidden Valley model.


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AALTONEN 2012AB looked in 5.1 fb**-1 of p pbar collisions at sqrt(s) = 1.96 TeV for anomalous production of multiple low-energy leptons in association with a W or Z boson. Such events may occur in hidden valley models in which a supersymmetric Higgs boson is produced in association with a W or Z boson, with H --> chitilde_1()0 chitilde_1()0 pair and with the chitilde_{{1}}()0 further decaying into a dark photon (gamma_{{D}}) and the unobservable lightest SUSY particle of the hidden sector. As the gamma_{{D}} is expected to be light, it may decay into a lepton pair. No significant excess over the SM expectation is observed and a limit at 95% C.L. is set on the cross section for a benchmark model of supersymmetric hidden-valley Higgs production.


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AAD 2011AA looked in 34 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with >=4 jets originating from pair production of scalar gluons, each decaying to two gluons. No two-jet resonances are observed over the SM background. Limits are derived on the cross section times branching ratio (see Fig. 3). Assuming 100% branching ratio for the decay to two gluons, the quoted exclusion range is obtained, except for a 5 GeV mass window around 140 GeV.


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CHATRCHYAN 2011E looked in 35 pb**-1 of p p collisions at sqrt(s) = 7 TeV for events with collimated mu pairs (leptonic jets) from the decay of hidden sector states. No evidence for new resonance production is found. Limits are derived and compared to various SUSY models (see Fig. 4) where the LSP, either the chitilde_{{1}}()0 or a qtilde, decays to dark sector particles.


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ABAZOV 2010N looked in 5.8 fb**-1 of p pbar collisions at sqrt(s) = 1.96 TeV for events from hidden valley models in which a chitilde_{{1}}^0() decays into a dark photon, gamma_{{D}}, and the unobservable lightest SUSY particle of the hidden sector. As the gamma_{{D}} is expected to be light, it may decay into a tightly collimated lepton pair, called lepton jet. They searched for events with notET and two isolated lepton jets observable by an opposite charged lepton pair e e, e mu or mu mu. No significant excess over the SM expectation is observed, and a limit at 95% C.L. on the cross section times branching ratio is derived, see their Table I. They also examined the invariant mass of the lepton jets for a narrow resonance, see their Fig. 4, but found no evidence for a signal.


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AAD 2020AM search for a top-color Z^' decaying to t tbar in p p collisions at sqrt(s) = 13 TeV. The quoted limit is for width(Z^')/M(Z^') = 0.01. The limit becomes M(Z^') > 4700 GeV for width(Z^')/M(Z^') = 0.03.


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AAD 2020W search for techni-rho decaying to pi_T W in p p collisions at sqrt(s) = 13 TeV. See their Fig. 5a for limits on.


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AAD 2016W search for color octet vector resonance decaying to b B in p p collisions at sqrt(s) = 8 TeV. The vector like quark B is assumed to decay to b H. See their Fig.3 and Fig.4 for limits on sigma.B.


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KHACHATRYAN 2016E search for top-color Z^' decaying to t tbar. The quoted limit is for width(Z^')/mass(Z^') = 0.012. Also exclude mass(Z^') < 2.9 TeV for wider topcolor Z^' with width(Z^')/mass(Z^') = 0.1.


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AAD 2015AB search for long-lived hidden valley pi_{{v}} particles which are produced in pairs by the decay of a scalar boson. pi_{{v}} is assumed to decay into dijets. See their Fig. 10 for the limit on sigmaB.


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AAD 2015AO search for top-color Z^' decaying to t tbar. The quoted limit is for width(Z^')/mass(Z^') = 0.012.


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AAD 2015BB search for minimal walking technicolor (MWT) isotriplet vector and axial-vector resonances decaying to W h or Z h. See their Fig. 3 for the exclusion limit in the MWT parameter space.


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AAD 2015Q search for long-lived hidden valley pi_{{v}} particles which are produced in pairs by the decay of scalar boson. pi_{{v}} is assumed to decay into dijets. See their Fig. 5 and Fig. 6 for the limit on sigmaB.


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AAIJ 2015AN search for long-lived hidden valley pi_{{v}} particles which are produced in pairs by the decay of scalar boson with a mass of 120GeV. pi_{{v}} is assumed to decay into dijets. See their Fig. 4 for the limit on sigma B.


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KHACHATRYAN 2015C search for a vector techni-resonance decaying to W Z. The limit assumes M(pi_{{T}}) = (3/4) M(rho_{{T}}) - 25 GeV. See their Fig.3 for the limit in M(pi_{{T}})-M(rho_{{T}}) plane of the low scale technicolor model.


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KHACHATRYAN 2015W search for long-lived hidden valley pi_{{v}} particles which are produced in pairs in the decay of heavy higgs boson H. pi_{{v}} is assumed to decay into lepton+ lepton-. See their Fig. 7 and Fig. 8 for the limits on sigma B.


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AAD 2014AT search for techni-omega and techni-a resonances decaying to V gamma with V = W(lepton nu) or Z(lepton+ lepton-).


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AAD 2014V search for vector techni-resonances decaying into electron or muon pairs in p p collisions at sqrt(s) = 8 TeV. See their table IX for exclusion limits with various assumptions.


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CHATRCHYAN 2013AP search for top-color leptophobic Z^' decaying to t tbar. The quoted limit is for width(Z^')/mass(Z^') = 0.012.


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BAAK 2012 give electroweak oblique parameter constraints on the QCD-like technicolor models. See their Fig. 28.


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CHATRCHYAN 2012AF search for a vector techni-resonance decaying to W Z. The limit assumes M(pi_{{T}})= (3/4) M(rho_{{T}})- 25 GeV. See their Fig. 3 for the limit in M(pi_{{T}})-M (rho_{{T}}) plane of the low scale technicolor model.


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Using the LHC limit on the Higgs boson production cross section, CHIVUKULA 2011 obtain a limit on the top-Higgs mass > 300 GeV at 95% CL assuming 150 GeV top-pion mass.


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Using the LHC limit on the Higgs boson production cross section, CHIVUKULA 2011A obtain a limit on the techinipion mass ruling out the region 110 GeV < mass(P) < 2mass(t). Existence of color techni-fermions, top-color mechanism, and N_{{TC}}() >= 3 are assumed.


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AALTONEN 2010I search for the vector techni-resonances (rho_{{T}}, omega_{{T}}) decaying into W pi_T with W --> lepton nu and pi_T --> b bbar, b cbar, or b ubar. See their Fig. 3 for the exclusion plot in M(pi_{{T}})-M(rho_{{T}}) plane.


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ABAZOV 2010A search for a vector techni-resonance decaying into W Z. The limit assumes M(rho_{{T}})< M(pi_{{T}}) + M(W).


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ABAZOV 2007I search for the vector techni-resonances (rho_{{T}}, omega_{{T}}) decaying into W pi_T with W --> e nu and pi_T --> b bbar or b cbar. See their Fig. 2 for the exclusion plot in M(pi_{{T}})-M(rho_{{T}}) plane.


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ABULENCIA 2005A search for resonances decaying to electron or muon pairs in p pbar collisions. at sqrt(s) = 1.96 TeV. The limit assumes Technicolor-scale mass parameters M_{{V}} = M_{{A}} = 500 GeV.


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CHEKANOV 2002B search for color octet techni-pi P decaying into dijets in e p collisions. See their Fig. 5 for the limit on sigma(e p --> e P X).B(P --> 2j).


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ABAZOV 2001B searches for vector techni-resonances (rho_{{{T}}},omega_{{{T}}}) decaying to e+ e-. The limit assumes M(rho_{{{T}}}) = M(omega_{{{T}}}) <M(pi_{{{T}}})+M(W).


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The limit is independent of the pi_{{{T}}} mass. See their Fig. 9 and Fig. 10 for the exclusion plot in the M(rho_{{{T}}})-M(pi_{{{T}}}) plane. ABDALLAH 2001 limit on the techni-pion mass is M(pi_{{{T}}})>79.8 GeV for N(D)=2, assuming its point-like coupling to gauge bosons.


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AFFOLDER 2000F search for rho_{{{T}}} decaying into W pi_T or pi_T pi_T with W --> lepton nu and pi_T --> bbar b, bbar c. See Fig. 1 in the above Note on ``Dynamical Electroweak Symmetry Breaking'' for the exclusion plot in the M(rho_{{{T}}})-M(pi_{{{T}}}) plane.


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AFFOLDER 2000K search for the rho_{{{T8}}} decaying into pi_LQ pi_LQ with pi_LQ --> b nu. For pi_LQ --> c nu, the limit is M(rho_{{{T8}}})>510 GeV. See their Fig. 2 and Fig. 3 for the exclusion plot in the M(rho_{{{T8}}})-M(pi_{{LQ}}) plane.


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ABE 1999F search for a new particle X decaying into b bbar in p pbar collisions at Ecm= 1.8 TeV. See Fig. 7 in the above Note on ``Dynamical Electroweak Symmetry Breaking'' for the upper limit on sigma(p pbar --> X)*B(X --> b bbar). ABE 1999F also exclude top gluons of width Gamma=0.3M in the mass interval 280<M<670 GeV, of width Gamma=0.5M in the mass interval 340<M<640 GeV, and of width Gamma=0.7M in the mass interval 375<M<560 GeV.


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ABE 1999N search for the techni-omega decaying into gamma pi_T. The technipion is assumed to decay pi_T --> b bbar. See Fig. 2 in the above Note on ``Dynamical Electroweak Symmetry Breaking'' for the exclusion plot in the M(omega_{{{T}}})-M(pi_{{{T}}}) plane.


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ABE 1997G search for a new particle X decaying into dijets in p pbar collisions at Ecm= 1.8 TeV. See Fig. 5 in the above Note on ``Dynamical Electroweak Symmetry Breaking'' for the upper limit on sigma(p pbar --> X)*B(X --> 2j).


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BABICH 2003 obtain a bound -0.175 TeV**-2<1/Lambda(LL)**2 <0.095 TeV**-2 (95%CL) in a model independent analysis allowing all of Lambda(LL), Lambda(LR), Lambda(RL), Lambda(RR) to coexist.


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AABOUD 2017AT limits are from p p collisions at sqrt(s) = 13 TeV. The quoted limit uses a uniform positive prior in 1/Lambda^2.


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AAD 2021AU search for new phenomena in final states with e+ e- and one or no b-tagged jets in p p collisions at sqrt(s) = 13 TeV. The quoted limits assume g_{{*}}^2 = 4 pi.


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AAD 2021Q limits are from p p collisions at sqrt(s) = 13 TeV. A frequentist statistical framework is used to remove the prior dependence.


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AABOUD 2016U limits are from p p collisions at sqrt(s) = 13 TeV. The quoted limit uses a uniform positive prior in 1/Lambda^2.


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AAD 2014BE limits are from p p collisions at sqrt(s) = 8 TeV. The quoted limit uses a uniform positive prior in 1/Lambda^2.


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ABDALLAH 2011 limit is from e+ e- --> t cbar cross section. Lambda_{{LL}} = Lambda_{{LR}} = Lambda_{{RL}} = Lambda_{{RR}} is assumed.


pdgid: S054CTS
text:
AAD 2021AU search for new phenomena in final states with mu+ mu- and one or no b-tagged jets in p p collisions at sqrt(s) = 13 TeV. The quoted limits assume g_{{*}}^2 = 4 pi.


pdgid: S054CTN
text:
JODIDIO 1986 limit is from mu+ --> nubar_mu e+ nu_e. Chirality invariant interactions L = (g**2/Lambda**2) [eta(LL) (nubar_{{mu L}}gamma**alphamu_{{L}}) (ebar_{{L}}gamma(alpha)nu_{{e L}}) + eta_{{LR}} (nubar_{{mu L}}gamma**alphanu_{{e L}} (ebar_{{R}}gamma_{{alpha}}mu_{{R}})] with g**2/4pi = 1 and (eta(LL),eta(LR)) = (0,+-1) are taken. No limits are given for Lambda(LL)**+- with (eta(LL),eta(LR)) = (+-1,0). For more general constraints with right-handed neutrinos and chirality nonconserving contact interactions, see their text.


pdgid: S054CTN
text:
DIAZCRUZ 1994 limits are from Gamma(tau --> e nu nu) and assume flavor-dependent contact interactions with Lambda(tau nu_tau e nu_e)<<Lambda(mu nu_mu e nu_e).


pdgid: S054CTN
text:
DIAZCRUZ 1994 limits are from Gamma(tau --> mu nu nu) and assume flavor-dependent contact interactions with Lambda(tau nu_tau mu nu_mu)<<Lambda(mu nu_mu e nu_e).


pdgid: S054CTQ
text:
AABOUD 2017AK limit is from dijet angular distribution in p p collisions at sqrt(s) = 13 TeV. u, d, and s quarks are assumed to be composite.


pdgid: S054CTQ
text:
AABOUD 2018AV obtain limit on t_{{R}} compositeness 2pi/Lambda_{{RR}}^2 < 1.6 TeV**-2 at 95% CL from t tbar t tbar production in the p p collisions at Ecm = 13 TeV.


pdgid: S054CTQ
text:
SIRUNYAN 2017F limit is from dijet angular cross sections in p p collisions at Ecm = 13 TeV. All quarks are assumed to be composite.


pdgid: S054CTQ
text:
AAD 2016S limit is from dijet angular selections in p p collisions at Ecm = 13 TeV. u, d, and s quarks are assumed to be composite.


pdgid: S054CTQ
text:
AAD 2015AR obtain limit on the t_{{R}} compositeness 2pi/Lambda_{{RR}}^2() < 6.6 TeV**-2 at 95% CL from the t tbar t tbar production in the p p collisions at Ecm = 8 TeV.


pdgid: S054CTQ
text:
AAD 2015BY obtain limit on the t_{{R}} compositeness 2pi/Lambda(RR)**2 < 15.1 TeV**-2 at 95% CL from the t tbar t tbar production in the p p collisions at Ecm = 8 TeV.


pdgid: S054CTQ
text:
AAD 2015L limit is from dijet angular distribution in p p collisions at Ecm = 8 TeV. u, d, and s quarks are assumed to be composite.


pdgid: S054CTQ
text:
KHACHATRYAN 2015J limit is from dijet angular distribution in p p collisions at Ecm = 8 TeV. u, d, s, c, and b quarks are assumed to be composite.


pdgid: S054CTQ
text:
FABBRICHESI 2014 obtain bounds on chromoelectric and chromomagnetic form factors of the top-quark using p p --> t tbar and p pbar --> t tbar cross sections. The quoted limit on the q qbar t tbar contact interaction is derived from their bound on the chromoelectric form factor.


pdgid: S054CTD
text:
AAD 2024AC limit is from the measurement of the t tbar production cross section with large missing notET in p p collisions at sqrt(s) = 13 TeV.


pdgid: S054EXP
text:
From e+ e- collisions at sqrt(s) = 189 -- 209 GeV. f = f^' is assumed. ACHARD 2003B also obtain limit for f = -f^': mass(e^*)>96.6 GeV.


pdgid: S054EXS
text:
SIRUNYAN 2020AJ search for e^* production in 2e 2j final states in p p collisions at sqrt(s) = 13 TeV. The quoted limit assumes Lambda = mass(e^*), f = f^' = 1. The contact interaction is included. See their Fig.11 for exclusion limits in mass(e^*)-Lambda plane.


pdgid: S054EXS
text:
AABOUD 2019AZ search for single e^* production in p p collisions at sqrt(s) = 13 TeV. The limit quoted above is from e^* --> e q qbar and e^* --> nu W decays assuming f = f^' = 1 and mass(e^*) = Lambda. The contact interaction is included in e^* production and decay amplitudes. See their Fig.6 for exclusion limits in mass(e^*)-Lambda plane.


pdgid: S054EXS
text:
SIRUNYAN 2019Z search for e^* production in lepton lepton gamma final states in p p collisions at sqrt(s) = 13 TeV. The quoted limit assumes Lambda = mass(e^*), f = f^' = 1. The contact interaction is included in the e^* production and decay amplitudes.


pdgid: S054EXS
text:
KHACHATRYAN 2016AQ search for single e^* production in p p collisions at sqrt(s) = 8 TeV. The limit above is from the e^* --> e gamma search channel assuming f = f^' = 1, mass(e^*) = Lambda. See their Table 7 for limits in other search channels or with different assumptions.


pdgid: S054EXS
text:
AAD 2015AP search for e^* production in evens with three or more charged leptons in p p collisions at sqrt(s) = 8 TeV. The quoted limit assumes Lambda = mass(e^*), f = f^' = 1. The contact interaction is included in the e^* production and decay amplitudes.


pdgid: S054EXS
text:
AAD 2013BB search for single e^* production in p p collisions with e^* --> e gamma decay. f = f^' = 1, and e^* production via contact interaction with Lambda = mass(e^*) are assumed.


pdgid: S054EXS
text:
CHATRCHYAN 2013AE search for single e^* production in p p collisions with e^* --> e gamma decay. f = f^' = 1, and e^* production via contact interaction with Lambda = mass(e^*) are assumed.


pdgid: S054EXS
text:
AAD 2012AZ search for e^* production via four-fermion contact interaction in p p collisions with e^* --> e gamma decay. The quoted limit assumes Lambda = mass(e^*). See their Fig. 8 for the exclusion plot in the mass-coupling plane.


pdgid: S054EXG
text:
ABDALLAH 2004N also obtain a limit on the excited electron mass with e e^* chiral coupling, mass(e^*)>295 GeV at 95% CL.


pdgid: S054EXI
text:
DORENBOSCH 1989 obtain the limit lambda(gamma)**2Lambda(cut)**2/mass**2(e^*) < 2.6 (95% CL), where Lambda(cut) is the cutoff scale, based on the one-loop calculation by GRIFOLS 1986. If one assumes that Lambda(cut) = 1 TeV and lambda_{{gamma}} = 1, one obtains mass(e^*) > 620 GeV. However, one generally expects lambda_{{gamma}} ~~ mass(e^*)/Lambda(cut) in composite models.


pdgid: S054EXI
text:
GRIFOLS 1986 uses nu_mu e --> nu_mu e and nubar_mu e --> nubar_mu e data from CHARM Collaboration to derive mass limits which depend on the scale of compositeness.


pdgid: S054EXI
text:
RENARD 1982 derived from g-2 data limits on mass and couplings of e^* and mu^*. See figures 2 and 3 of the paper.


pdgid: S054MXP
text:
From e+ e- collisions at sqrt(s) = 189 -- 209 GeV. f = f^' is assumed. ACHARD 2003B also obtain limit for f = -f^': mass(mu^*)>96.6 GeV.


pdgid: S054MXS
text:
SIRUNYAN 2020AJ search for mu^* production in 2mu 2j final states in p p collisions at sqrt(s) = 13 TeV. The quoted limit assumes Lambda = mass(mu^*), f = f^' = 1. The contact interaction is included. See their Fig.11 for exclusion limits in mass(mu^*)-Lambda plane.


pdgid: S054MXS
text:
SIRUNYAN 2019Z search for mu^* production in lepton lepton gamma final states in p p collisions at sqrt(s) = 13 TeV. The quoted limit assumes Lambda = mass(mu^*), f = f^' = 1. The contact interaction is included in the mu^* production and decay amplitudes.


pdgid: S054MXS
text:
AAD 2016BM search for mu^* production in mu mu j j events in p p collisions at sqrt(s) = 8 TeV. Both the production and decay are assumed to occur via a contact interaction with Lambda = mass(mu^*).


pdgid: S054MXS
text:
KHACHATRYAN 2016AQ search for single mu^* production in p p collisions at sqrt(s) = 8 TeV. The limit above is from the mu^* --> mu gamma search channel assuming f = f^' = 1, mass(mu^*) = Lambda. See their Table 7 for limits in other search channels or with  different assumptions.


pdgid: S054MXS
text:
AAD 2015AP search for mu^* production in evens with three or more charged leptons in p p collisions at sqrt(s) = 8 TeV. The quoted limit assumes Lambda = mass(mu^*), f = f^' = 1. The contact interaction is included in the mu^* production and decay amplitudes.


pdgid: S054MXS
text:
AAD 2013BB search for single mu^* production in p p collisions with mu^* --> mu gamma decay. f = f^' = 1, and mu^* production via contact interaction with Lambda = mass(mu^*) are assumed.


pdgid: S054MXS
text:
CHATRCHYAN 2013AE search for single mu^* production in p p collisions with mu^* --> mu gamma decay. f = f^' = 1, and mu^* production via contact interaction with Lambda = mass(mu^*) are assumed.


pdgid: S054MXS
text:
AAD 2012AZ search for mu^* production via four-fermion contact interaction in p p collisions with mu^* --> mu gamma decay. The quoted limit assumes Lambda = mass(mu^*). See their Fig. 8 for the exclusion plot in the mass-coupling plane.


pdgid: S054TXP
text:
From e+ e- collisions at sqrt(s) = 189 -- 209 GeV. f = f^' is assumed. ACHARD 2003B also obtain limit for f = -f^': mass(tau^*)>96.6 GeV.


pdgid: S054TXS
text:
AAD 2023BJ search for tau^* produced in association with tau and decaying into tau q qbar via a contact interaction with g(contact)**2 = (4pi)**2. The limit quoted above assumes Lambda = mass(tau^*).


pdgid: S054TXS
text:
AAD 2015AP search for tau^* production in events with three or more charged leptons in p p collisions at sqrt(s) = 8 TeV. The quoted limit assumes Lambda = mass(tau^*), f = f^' = 1. The contact interaction is included in the tau^* production and decay amplitudes.


pdgid: S054TXS
text:
ACHARD 2003B result is from e+ e- collisions at sqrt(s) = 189 -- 209 GeV. f = f^' = Lambda/mass(tau^*) is assumed. See their Fig. 4 for the exclusion plot in the mass-coupling plane.


pdgid: S054TXS
text:
ABBIENDI 2002G result is from e+ e- collisions at sqrt(s) = 183 -- 209 GeV. f = f^' = Lambda/mass(tau^*) is assumed for tau^* coupling. See their Fig. 4c for the exclusion limit in the mass-coupling plane.


pdgid: S054EXN
text:
AAD 2015AP search for nu^* pair production in evens with three or more charged leptons in p p collisions at sqrt(s) = 8 TeV. The quoted limit assumes Lambda = mass(nu^*), f = f^' = 1. The contact interaction is included in the nu^* production and decay amplitudes.


pdgid: S054EXN
text:
From e+ e- collisions at sqrt(s) = 192 -- 209 GeV, ABBIENDI 2004N obtain limit on CS(e+ e- --> nu^* nu^*) B**2(nu^* --> nu gamma). See their Fig.2. The limit ranges from 20 to 45 fb for mass(nu^*) > 45 GeV.


pdgid: S054EXN
text:
From e+ e- collisions at sqrt(s) = 189 -- 209 GeV. f = -f^' is assumed. ACHARD 2003B also obtain limit for f = f^': mass(nu_{{e}}^*)>101.7 GeV, mass(nu_{{mu}}^*)>101.8 GeV, and mass(nu_{{tau}}^*)>92.9 GeV. See their Fig. 4 for the exclusion plot in the mass-coupling plane.


pdgid: S054EXO
text:
AARON 2008 search for single nu^*() production in e p collisions with the decays nu^*() --> nu gamma, nu Z, e W. The quoted limit assumes f = -f^'() = Lambda/mass(nu^*()). See their Fig. 3 and Fig. 4 for the exclusion plots in the mass-coupling plane.


pdgid: S054EXO
text:
TUMASYAN 2023AL search for Majorana excited neutrino nu^* produced and decaying via gauge and contact interactions. The limit quoted above is for lepton = e with Lambda = M(nu^*). The limit becomes M(nu^*) > 6.1 TeV for lepton = mu.


pdgid: S054EXO
text:
ACHARD 2003B result is from e+ e- collisions at sqrt(s) = 189 -- 209 GeV. The quoted limit is for nu_{{e}}^*. f = -f^' = Lambda/mass(nu^*) is assumed. See their Fig. 4 for the exclusion plot in the mass-coupling plane.


pdgid: S054EXO
text:
ADLOFF 2002 search for single nu^* production in e p collisions with the decays nu^* --> nu gamma, nu Z, e W. The quoted limit assumes f = -f^' = Lambda/mass(nu^*). See their Fig. 1 for the exclusion plots in the mass-coupling plane.


pdgid: S054EXO
text:
CHEKANOV 2002D search for single nu^* production in e p collisions with the decays nu^* --> nu gamma, nu Z, e W. f = -f^' = Lambda/mass(nu^*) is assumed for the e^* coupling. CHEKANOV 2002D also obtain limit for f = f^' = Lambda/mass(nu^*): mass(nu^*)>135 GeV. See their Fig. 5c and Fig. 5d for the exclusion plot in the mass-coupling plane.


pdgid: S054EQP
text:
AALTONEN 2010H obtain limits on the q^*() q^*() production cross section in p pbar collisions. See their Fig. 3.


pdgid: S054EQP
text:
SIRUNYAN 2018V search for pair production of spin 3/2 excited top quarks. B(t_3/2^*() --> t g) = 1 is assumed.


pdgid: S054EQP
text:
BARATE 1998U obtain limits on the form factor. See their Fig. 16 for limits in mass-form factor plane.


pdgid: S054EQS
text:
TUMASYAN 2023AF limit quoted above assumes b g --> b^* production. The limit becomes mass(b^*) >  4 TeV if contact interaction is included in the b^* production cross section. See their Fig. 5 for limits on.


pdgid: S054EQS
text:
TUMASYAN 2023BC search for excited light flavor quark q^* in p p collisions at sqrt(s) = 13 TeV. f = 1.0 is assumed.


pdgid: S054EQS
text:
TUMASYAN 2023BC search for excited b quark b^* in p p collisions at sqrt(s) = 13 TeV. $b^*$ production via gauge interactions and f = 1.0 are assumed. The limit becomes $m_{b^*}>3.8$TeV if contact interaction is included in the $b^*$ production cross section.


pdgid: S054EQS
text:
AAD 2020T search for resonances decaying into dijets in p p collisions at sqrt(s) = 13 TeV. Assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1.


pdgid: S054EQS
text:
SIRUNYAN 2020AI search for resonances decaying into dijets in p p collisions at sqrt(s) = 13 TeV. Assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1.


pdgid: S054EQS
text:
AABOUD 2018AB assume Lambda = mass(b^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in b^* production and decay amplitudes.


pdgid: S054EQS
text:
AABOUD 2018BA search for first-generation excited quarks (u^* and d^*) with degenerate mass, assuming Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
SIRUNYAN 2018AG search for first-generation excited quarks (u^* and d^*) with degenerate mass, assuming Lambda = mass(q^*), f_{{s}} = f = f^' = 1.


pdgid: S054EQS
text:
SIRUNYAN 2018BO assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
AABOUD 2017AK assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes. Only the decay of q^* --> g u and q^* --> g d is simulated as the benchmark signals in the analysis.


pdgid: S054EQS
text:
HAYRAPETYAN 2024G search for singly produced narrow resonances decaying to j j j in p p collisions at sqrt(s) = 13 TeV. See their Fig. 3 for limits on.


pdgid: S054EQS
text:
TUMASYAN 2022O search for b^* decaying to t W in p p collisions at sqrt(s) = 13  TeV. The limit quoted above assumes kappa_{{L}}^b = g_{{L}} = 1, kappa_{{R}}^b = g_{{R}} = 0. The  limit becomes mass(b^*) > 3.0 TeV (>3.2 TeV) if we assume kappa_{{L}}^b = g_{{L}} = 0,  kappa_{{R}}^b = g_{{R}} = 1 (kappa_{{L}}^b = g_{{L}} = 1, kappa_{{R}}^b = g_{{R}} = 1). See their  Fig. 3 for limits on.


pdgid: S054EQS
text:
SIRUNYAN 2021AG search for b^* decaying to t W in p p collisions at sqrt(s) = 13 TeV. The limit quoted above assumes kappa_{{L}}^b = g_{{L}} = 1, kappa_{{R}}^b = g_{{R}} = 0. The limit becomes mass(b^*) > 2.8 TeV (> 3.1 TeV) if we assume kappa_{{L}}^b = g_{{L}} = 0, kappa_{{R}}^b = g_{{R}} = 1 (kappa_{{L}}^b = g_{{L}} = kappa_{{R}}^b = g_{{R}} = 1). See their Fig. 5 for limits on.


pdgid: S054EQS
text:
KHACHATRYAN 2017W assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
AABOUD 2016 assume Lambda = mass(b^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in the b^* production and decay amplitudes.


pdgid: S054EQS
text:
AAD 2016AH search for b^* decaying to t W in p p collisions at sqrt(s) = 8 TeV. f_{{g}} = f_{{L}} = f_{{R}} = 1 are assumed. See their Fig. 12b for limits on sigma.B.


pdgid: S054EQS
text:
AAD 2016AV search for single production of vector-like quarks decaying to W b in p p collisions. See their Fig. 8 for the limits on couplings and mixings.


pdgid: S054EQS
text:
AAD 2016S assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
KHACHATRYAN 2016I search for b^* decaying to t W in p p collisions at sqrt(s) = 8 TeV. kappa_{{L}}^b() = g_{{L}} = 1, kappa_{{R}}^b() = g_{{R}} = 0 are assumed. See their Fig. 8 for limits on sigma B.


pdgid: S054EQS
text:
KHACHATRYAN 2016K assume Lambda = mass(q^*), f_{{s}} = f = f^'= 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
KHACHATRYAN 2016L search for resonances decaying to dijets in p p collisions at sqrt(s) = 8 TeV using the data scouting technique which increases the sensitivity to the low mass resonances.


pdgid: S054EQS
text:
AAD 2015V assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact  interactions are not included in q^* production and decay amplitudes.


pdgid: S054EQS
text:
KHACHATRYAN 2015V assume Lambda = mass(q^*), f_{{s}} = f = f^' = 1. The contact interactions are not included in q^* production and decay amplitudes.


pdgid: S054CQ
text:
ABE 1989D look for pair production of unit-charged particles which leave the detector before decaying. In the above limit the color sextet quark is assumed to fragment into a unit-charged or neutral hadron with equal probability and to have long enough lifetime not to decay within the detector. A limit of 121 GeV is obtained for a color decuplet.


pdgid: S054CL
text:
ABE 1989D look for pair production of unit-charged particles which leave the detector before decaying. In the above limit the color octet lepton is assumed to fragment into a unit-charged or neutral hadron with equal probability and to have long enough lifetime not to decay within the detector. The limit improves to 99 GeV if it always fragments into a unit-charged hadron.


pdgid: S054CL
text:
ABT 1993 search for e_{{8}} production via e-gluon fusion in e p collisions with e_8 --> e g. See their Fig. 3 for exclusion plot in the mass(e_{{8}})--Lambda plane for mass(e_{{8}}) = 35 -- 220 GeV.


pdgid: S054CN
text:
BARGER 1989 used ABE 1989B limit for events with large missing transverse momentum. Two-body decay nu_8 --> nu g is assumed.


pdgid: S054CN
text:
BARTEL 1987B is at Ecm = 46.3-46.78 GeV. The limit assumes the nu_{{8}} pair production cross section to be eight times larger than that of the corresponding heavy neutrino pair production. This assumption is not valid in general for the weak couplings, and the limit can be sensitive to its SU(2)(L)xU(1)(Y) quantum numbers.


pdgid: S071DGF
text:
BLAKEMORE 2021 obtain constraints on non-Newtonian forces with strengths |alpha| ~> E8 and length scales R > 10 mum. See their Fig. 4 for more details including comparison with previous searches.


pdgid: S071DGF
text:
HEACOCK 2021 obtain constraints on non-Newtonian forces with strengths E18~< |alpha|~< E25 and length scales R ~= 0.02 -- 10 nm. See their Figure 3 for more details. This improves the results of HADDOCK 2018. These constraints do not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
LEE 2020 search for new forces probing a range of |alpha| ~=  and length scales R ~= 7 -- 90 mum. For delta = 1 the bound on R is 30 mum. See their Fig. 5 for details on the bound.


pdgid: S071DGF
text:
TAN 2020A search for new forces probing a range of |alpha| ~= 4E-3 -- 1E2 and length scales R ~= 40 -- 350 mum. See their Fig. 6 for details on the bound.


pdgid: S071DGF
text:
BERGE 2018 uses results from the MICROSCOPE experiment to obtain constraints on non-Newtonian forces with strengths E-11~< |alpha|~< E-7 and length scales R ~>E5 m. See their Figure 1 for more details. These constraints do not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
FAYET 2018A uses results from the MICROSCOPE experiment to obtain constraints on an EP-violating force possibly arising from a new U(1) gauge boson. For R ~>E7 m the limits are |alpha| ~< a few E-13 to a few E-11 depending on the coupling, corresponding to |epsilon| ~< E-24 for the coupling of the new spin-1 or spin-0 mediator. These constraints do not place limits on the size of extra flat dimensions. This extends the results of FAYET 2018.


pdgid: S071DGF
text:
KLIMCHITSKAYA 2017A uses an experiment that measures the difference of Casimir forces to obtain bounds on non-Newtonian forces with strengths |alpha| ~= E5 -- E17 and length scales R = 0.03 -- 10 mum. See their Fig. 3. These constraints do not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
XU 2013 obtain constraints on non-Newtonian forces with strengths |alpha| ~= 10**34 -- 10**36 and length scales R ~= 1 -- 10 fm. See their Fig. 4 for more details. These constraints do not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
BEZERRA 2011 obtain constraints on non-Newtonian forces with strengths E11~< |alpha|~< E18 and length scales R = 30 -- 1260 nm. See their Fig. 2 for more details. These constraints do not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
SUSHKOV 2011 obtain improved limits on non-Newtonian forces with strengths E7~< |alpha| ~< E11 and length scales 0.4 mum < R < 4 mum (95% CL). See their Fig. 2. These bounds do not place limits on the size of extra flat dimensions. However, a model dependent bound of M_{{*}} > 70 TeV is obtained assuming gauge bosons that couple to baryon number also propagate in (4 + delta) dimensions.


pdgid: S071DGF
text:
BEZERRA 2010 obtain improved constraints on non-Newtonian forces with strengths E19~< |alpha|~< E29 and length scales R = 1.6 -- 14 nm (95% CL). See their Fig. 1. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
MASUDA 2009 obtain improved constraints on non-Newtonian forces with strengths E9~<|alpha|~<E11 and length scales R = 1.0 -- 2.9 mum (95% CL). See their Fig. 3. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
GERACI 2008 obtain improved constraints on non-Newtonian forces with strengths |alpha| > 14,000 and length scales R = 5 -- 15 micrometers. See their Fig. 9. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
TRENKEL 2008 uses two independent measurements of Newton's constant G to constrain new forces with strength |alpha|~=E-4 and length scales R = 0.02 -- 1 m. See their Fig. 1. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
DECCA 2007A search for new forces and obtain bounds in the region with strengths |alpha| ~= E13 -- E18 and length scales R = 20 -- 86 nm. See their Fig. 6. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
KAPNER 2007 search for new forces, probing a range of |alpha| ~= 10**-3 -- 10**5 and length scales R ~= 10 -- 1000 mum. For delta = 1 the bound on R is 44 mum. For delta = 2, the bound is expressed in terms of M_{{*}}, here translated to a bound on the radius. See their Fig. 6 for details on the bound.


pdgid: S071DGF
text:
TU 2007 search for new forces probing a range of |alpha| ~= E-1 -- E5 and length scales R ~= 20 -- 1000 mum. For delta = 1 the bound on R is 53 mum. See their Fig. 3 for details on the bound.


pdgid: S071DGF
text:
SMULLIN 2005 search for new forces, and obtain bounds in the region with strengths alpha ~= 10**3 -- 10**8 and length scales R = 6 -- 20 mum. See their Figs. 1 and 16 for details on the bound. This work does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
HOYLE 2004 search for new forces, probing alpha down to 10**-2 and distances down to 10mum. Quoted bound on R is for delta = 2. For delta = 1, bound goes to 160 mum. See their Fig. 34 for details on the bound.


pdgid: S071DGF
text:
CHIAVERINI 2003 search for new forces, probing alpha above 10**4 and lambda down to 3mum, finding no signal. See their Fig. 4 for details on the bound. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071DGF
text:
LONG 2003 search for new forces, probing alpha down to 3, and distances down to about 10mum. See their Fig. 4 for details on the bound.


pdgid: S071DGF
text:
HOYLE 2001 search for new forces, probing alpha down to 10**-2 and distances down to 20mum. See their Fig. 4 for details on the bound. The quoted bound is for alpha >= 3.


pdgid: S071DGF
text:
HOSKINS 1985 search for new forces, probing distances down to 4 mm. See their Fig. 13 for details on the bound. This bound does not place limits on the size of extra flat dimensions.


pdgid: S071OS6
text:
AAD 2021F search for p p --> j G, using 139 fb**-1 of data at sqrt(s) = 13 TeV to place lower limits on M_{{D}} for two to six extra dimensions (see their Table X), from which this bound on R is derived. This limit supersedes that in AABOUD 2018I.


pdgid: S071OS6
text:
HANNESTAD 2003 obtain a limit on R from the heating of old neutron stars by the surrounding cloud of trapped KK gravitons. Limits for all delta<=7 are given in their Tables V and VI. These limits supersede those in HANNESTAD 2002.


pdgid: S071OS6
text:
SIRUNYAN 2021A search for p p --> Z G, using 137 fb**-1 of data at sqrt(s) = 13 TeV to place lower limits on M_{{D}} for two to seven extra dimensions (see their Figure 12), from which this bound on R is derived. These limits supersede those obtained in SIRUNYAN 2018BV.


pdgid: S071OS6
text:
TUMASYAN 2021D search for p p --> j G, using 137 fb**-1 of data at sqrt(s) = 13 TeV  to place lower limits on M_{{D}} for two to seven extra dimensions (see their Table 3), from which  this bound on R is derived. This limit supersedes that in SIRUNYAN 2018S.


pdgid: S071OS6
text:
SIRUNYAN 2017AQ search for p p --> gamma G, using 12.9 fb**-1 of data at sqrt(s) = 13 TeV to place limits on M_{{D}} for three to six extra dimensions (see their Table 3).


pdgid: S071OS6
text:
AABOUD 2016F search for p p --> gamma G, using 3.2 fb**-1 of data at sqrt(s) = 13 TeV to place limits on M_{{D}} for two to six extra dimensions (see their Figure 9), from which this bound on R is derived.


pdgid: S071OS6
text:
KHACHATRYAN 2016N search for p p --> gamma G, using 19.6 fb**-1 of data at sqrt(s) = 8 TeV to place limits on M_{{D}} for three to six extra dimensions (see their Table 5).


pdgid: S071OS6
text:
AAD 2015CS search for p p --> gamma G, using 20.3 fb**-1 of data at sqrt(s) = 8 TeV  to place lower limits on M_{{D}} for two to six extra dimensions (see their Fig. 18).


pdgid: S071OS6
text:
AAD 2013C search for p p --> gamma G, using 4.6 fb**-1 of data at sqrt(s) = 7 TeV to place bounds on M_{{D}} for two to six extra dimensions, from which this bound on R is derived.


pdgid: S071OS6
text:
AAD 2013D search for the dijet decay of quantum black holes in 4.8 fb**-1 of data produced in p p collisions at sqrt(s) = 7 TeV to place bounds on M_{{D}} for two to seven extra dimensions, from which these bounds on R are derived. Limits on M_{{D}} for all delta <= 7 are given in their Table 3.


pdgid: S071OS6
text:
AJELLO 2012 obtain a limit on R from the gamma-ray emission of point gamma sources that arise from the photon decay of KK gravitons which are gravitationally bound around neutron stars. Limits for all delta <= 7 are given in their Table 7.


pdgid: S071OS6
text:
AALTONEN 2008AC search for p pbar --> gamma G and p pbar --> j G at sqrt(s) = 1.96 TeV with 2.0 fb**-1 and 1.1 fb**-1 respectively, in order to place bounds on the fundamental scale and size of the extra dimensions. See their Table III for limits on all delta<= 6.


pdgid: S071OS6
text:
ABAZOV 2008S search for p pbar --> gamma G, using 1 fb**-1 of data at sqrt(s) = 1.96 TeV to place bounds on M_{{D}} for two to eight extra dimensions, from which these bounds on R are derived. See their paper for intermediate values of delta.


pdgid: S071OS6
text:
DAS 2008 obtain a limit on R from Kaluza-Klein graviton cooling of SN1987A due to plasmon-plasmon annihilation.


pdgid: S071OS6
text:
ABULENCIA,A 2006 search for p pbar --> j G using 368 pb**-1 of data at sqrt(s) = 1.96 TeV. See their Table II for bounds for all delta <= 6.


pdgid: S071OS6
text:
ABDALLAH 2005B search for e+ e- --> gamma G at sqrt(s) = 180 -- 209~GeV to place bounds on the size of extra dimensions and the fundamental scale. Limits for all delta <= 6 are given in their Table~6. These limits supersede those in ABREU 2000Z.


pdgid: S071OS6
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ACHARD 2004E search for e+ e- --> gamma G at sqrt(s) = 189 -- 209~GeV to place bounds on the size of extra dimensions and the fundamental scale. See their Table~8 for limits with delta <= 8. These limits supersede those in ACCIARRI 1999R.


pdgid: S071OS6
text:
ACOSTA 2004C search for pbar p --> j G at sqrt(s) = 1.8~TeV to place bounds on the size of extra dimensions and the fundamental scale. See their paper for bounds on delta~=~4,~6.


pdgid: S071OS6
text:
CASSE 2004 obtain a limit on R from the gamma-ray emission of point gamma sources that arises from the photon decay of gravitons around newly born neutron stars, applying the technique of HANNESTAD 2003 to neutron stars in the galactic bulge. Limits for all delta<=7 are given in their Table~I.


pdgid: S071OS6
text:
ABAZOV 2003 search for p pbar --> j G at sqrt(s)=1.8 TeV to place bounds on M(D) for 2 to 7 extra dimensions, from which these bounds on R are derived. See their paper for bounds on intermediate values of delta. We quote results without the approximate NLO scaling introduced in the paper.


pdgid: S071OS6
text:
HANNESTAD 2003 obtain a limit on R from graviton cooling of supernova SN1987a. Limits for all delta<=7 are given in their Tables V and VI.


pdgid: S071OS6
text:
HANNESTAD 2003 obtain a limit on R from gravitons emitted in supernovae and which subsequently decay, contaminating the diffuse cosmic gamma background. Limits for all delta<=7 are given in their Tables V and VI. These limits supersede those in HANNESTAD 2002.


pdgid: S071OS6
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HANNESTAD 2003 obtain a limit on R from gravitons emitted in two recent supernovae and which subsequently decay, creating point gamma sources. Limits for all delta<=7 are given in their Tables V and VI. These limits are corrected in the published erratum.


pdgid: S071OS6
text:
HEISTER 2003C use the process e+ e- --> gamma G at sqrt(s) = 189 -- 209 GeV to place bounds on the size of extra dimensions and the scale of gravity. See their Table 4 for limits with delta<=6 for derived limits on M(D).


pdgid: S071OS6
text:
AABOUD 2016D search for p p --> j G, using 3.2 fb**-1 of data at sqrt(s) = 13 TeV to FAIRBAIRN 2001 obtains bounds on R from over production of KK gravitons in the early universe. Bounds are quoted in paper in terms of fundamental scale of gravity. place lower limits on M_{{D}} for two to six extra dimensions (see their Table X), from which this Bounds depend strongly on temperature of QCD phase transition and range from bound on R is derived. R<0.13 mum to 0.001 mum for delta=2; bounds for delta=3,4 can be derived from Table 1 in the paper.


pdgid: S071OS6
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HANHART 2001 obtain bounds on R from limits on graviton cooling of supernova SN 1987a using numerical simulations of proto-neutron star neutrino emission.


pdgid: S071OS6
text:
CASSISI 2000 obtain rough bounds on M(D) (and thus R) from red giant cooling for delta=2,3. See their paper for details.


pdgid: S071OS6
text:
ACCIARRI 1999S search for e+ e- --> Z G at sqrt(s)=189 GeV. Limits on the gravity scale are found in their Table 2, for delta<=4.


pdgid: S071GEX
text:
SIRUNYAN 2018DD use dijet angular distributions in 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to place a lower bound on Lambda_{{T}}, here converted to M_{{TT}}. This updates the results of SIRUNYAN 2017F.


pdgid: S071GEX
text:
GIUDICE 2003 place bounds on Lambda(6), the coefficient of the gravitationally-induced dimension-6 operator (2pilambda/Lambda(6)**2)(Sumfbargamma(mu)gamma**5f)(Sumfbargamma**mugamma**5f), using data from a variety of experiments. Results are quoted for lambda=+-1 and are independent of delta.


pdgid: S071GEX
text:
HAYRAPETYAN 2024AJ use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to place lower limits on M_{{TT}}() (equivalent to their M_{{S}}). This updates the results of SIRUNYAN 2018DU.


pdgid: S071GEX
text:
SIRUNYAN 2021N use 137 (140) fb**-1 of data from p p collisions at sqrt(s) = 13 TeV in the dielectron (dimuon) channels to place a lower limit on Lambda_{{T}}, here converted to M_{{TT}}. Bounds on individual channels can be found in their Table 7.


pdgid: S071GEX
text:
SIRUNYAN 2019AC use 35.9 (36.3) fb**-1 of data from p p collisions at sqrt(s) = 13 TeV in the dielectron (dimuon) channels to place a lower limit on Lambda_{{T}}, here converted to M_{{TT}}. The dielectron and dimuon channels are combined with previous results in the diphoton channel to set the best limit. Bounds on individual channels and different priors can be found in their Table 2. This updates the results in KHACHATRYAN 2015AE.


pdgid: S071GEX
text:
AABOUD 2017AP use 36.7 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to place lower limits on M_{{TT}}() (equivalent to their M_{{S}}). This updates the results of AAD 2013AS.


pdgid: S071GEX
text:
AAD 2014BE use 20 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV in the dilepton channel to place lower limits on M_{{TT}}() (equivalent to their M_{{S}}).


pdgid: S071GEX
text:
AAD 2013E use 4.9 and 5.0 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV in the dielectron and dimuon channels, respectively, to place lower limits on M_{{TT}}() (equivalent to their M_{{S}}). The dielectron and dimuon channels are combined with previous results in the diphoton channel to set the best limit. Bounds on individual channels and different priors can be found in their Table VIII.


pdgid: S071GEX
text:
BAAK 2012 use electroweak precision observables to place bounds on the ratio Lambda_{{T}}/M_{{D}} as a function of M_{{D}}. See their Fig. 22 for constraints with a Higgs mass of 120 GeV.


pdgid: S071GEX
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AARON 2011C search for deviations in the differential cross section of e()+- p --> e()+- X in 446 pb**-1 of data taken at sqrt(s) = 301 and 319 GeV to place a bound on M_{{TT}}.


pdgid: S071GEX
text:
ABAZOV 2009AE use dijet angular distributions in 0.7 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place lower bounds on Lambda(T) (equivalent to their M(S)), here converted to M(TT).


pdgid: S071GEX
text:
ABAZOV 2009D use 1.05 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place lower bounds on Lambda_{{T}} (equivalent to their M_{{s}}), here converted to M_{{TT}}.


pdgid: S071GEX
text:
SCHAEL 2007A use e+ e- collisions at sqrt(s) = 189 -- 209 GeV to place lower limits on Lambda_{{T}}, here converted to limits on M_{{TT}}.


pdgid: S071GEX
text:
ABDALLAH 2006C use e+ e- collisions at sqrt(s)~130 -- 207 GeV to place lower limits on M_{{TT}}, which is equivalent to their definition of M_{{s}}. Bound shown includes all possible final state leptons, lepton = e, mu, tau. Bounds on individual leptonic final states can be found in their Table 31.


pdgid: S071GEX
text:
GERDES 2006 use 100 to 110 pb**-1 of data from p pbar collisions at sqrt(s) = 1.8 TeV, as recorded by the CDF Collaboration during Run I of the Tevatron. Bound shown includes a K-factor of 1.3. Bounds on individual e+ e- and gamma gamma final states are found in their Table I.


pdgid: S071GEX
text:
ABAZOV 2005V use 246 pb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to search for deviations in the differential cross section to mu+ mu- from graviton exchange.


pdgid: S071GEX
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CHEKANOV 2004B search for deviations in the differential cross section of e+- p --> e+- X with 130~pb^{-1} of combined data and Q^2 values up to 40,000~GeV**2 to place a bound on M(TT).


pdgid: S071GEX
text:
ABBIENDI 2003D use e+ e- collisions at sqrt(s)=181 -- 209 GeV to place bounds on the ultraviolet scale M(TT), which is equivalent to their definition of M(s).


pdgid: S071GEX
text:
ACHARD 2003D look for deviations in the cross section for e+ e- --> Z Z from sqrt(s) = 200 -- 209 GeV to place a bound on M(TT).


pdgid: S071GEX
text:
ADLOFF 2003 search for deviations in the differential cross section of e+- p --> e+- X at sqrt(s)=301 and 319 GeV to place bounds on M(TT).


pdgid: S071GEX
text:
HEISTER 2003C use e+ e- collisions at sqrt(s)= 189 -- 209 GeV to place bounds on the scale of dim-8 gravitational interactions. Their M(s)**+- is equivalent to our M(TT) with lambda=+-1.


pdgid: S071GEX
text:
ACHARD 2002 search for s-channel graviton exchange effects in e+ e- --> gamma gamma at Ecm = 192 -- 209 GeV.


pdgid: S071GEX
text:
ABBOTT 2001 search for variations in differential cross sections to e+ e- and gamma gamma final states at the Tevatron.


pdgid: S071GEX
text:
ABREU 2000A search for s-channel graviton exchange effects in e+ e- --> gamma gamma at Ecm= 189 -- 202 GeV.


pdgid: S071GEX
text:
ABREU 2000S uses e+ e- collisions at sqrt(s)=183 and 189 GeV. Bounds on mu and tau individual final states given in paper.


pdgid: S071GEX
text:
CHANG 2000B derive 3sigma limit on M(TT) of (28,19,15) TeV for delta=(2,4,6) respectively assuming the presence of a torsional coupling in the gravitational action. Highly model dependent.


pdgid: S071GEX
text:
CHEUNG 2000 obtains limits from anomalous diphoton production at OPAL due to graviton exchange. Original limit for delta=4. However, unknown UV theory renders delta dependence unreliable. Original paper works in HLZ convention.


pdgid: S071GEX
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GRAESSER 2000 obtains a bound from graviton contributions to g-2 of the muon through loops of 0.29 TeV for delta=2 and 0.38 TeV for delta=4,6. Limits scale as lambda**1/2. However calculational scheme not well-defined without specification of high-scale theory. See the ``Extra Dimensions Review.''


pdgid: S071GEX
text:
HAN 2000 calculates corrections to gauge boson self-energies from KK graviton loops and constrain them using S and T. Bounds on M(TT) range from 0.5 TeV (delta=6) to 1.1 TeV (delta=2); see text. Limits have strong dependence, lambda**delta+2, on unknown lambda coefficient.


pdgid: S071GEX
text:
MATHEWS 2000 search for evidence of graviton exchange in CDF and D0 dijet production data. See their Table 2 for slightly stronger delta-dependent bounds. Limits expressed in terms of Mtilde(S)**4 = M(TT)**4/8.


pdgid: S071GEX
text:
MELE 2000 obtains bound from KK graviton contributions to e+ e- --> V V (V=gamma,W,Z) at LEP. Authors use Hewett conventions.


pdgid: S071GEX
text:
ABBIENDI 1999P search for s-channel graviton exchange effects in e+ e- --> gamma gamma at Ecm=189 GeV. The limits G(+)>660 GeV and G(-)>634 GeV are obtained from combined Ecm=183 and 189 GeV data, where G(+-) is a scale related to the fundamental gravity scale.


pdgid: S071GEX
text:
ACCIARRI 1999M search for the reaction e+ e- --> gamma G and s-channel graviton exchange effects in e+ e- --> gamma gamma, W+ W-, Z Z, e+ e-, mu+ mu-, tau+ tau-, q qbar at Ecm=183 GeV. Limits on the gravity scale are listed in their Tables 1 and 2.


pdgid: S071GEX
text:
ACCIARRI 1999s search for the reaction e+ e- --> Z G and s-channel graviton exchange effects in e+ e- --> gamma gamma, W+ W-, Z Z, e+ e-, mu+ mu-, tau+ tau-, q qbar at Ecm=189 GeV. Limits on the gravity scale are listed in their Tables 1 and 2.


pdgid: S071GEX
text:
BOURILKOV 1999 performs global analysis of LEP data on e+ e- collisions at sqrt(s)=183 and 189 GeV. Bound is on Lambda(T).


pdgid: S071KK
text:
AAD 2012CC use 4.9 and 5.0 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV in the dielectron and dimuon channels, respectively, to place a lower bound on the mass of the lightest KK Z/gamma boson (equivalent to 1/R = M_{{c}}). The limit quoted here assumes a flat prior corresponding to when the pure Z/gamma KK cross section term dominates. See their Section 15 for more details.


pdgid: S071KK
text:
BARBIERI 2004 use electroweak precision observables to place a lower bound on the compactification scale 1/R. Both the gauge bosons and the Higgs boson are assumed to propagate in the bulk.


pdgid: S071KK
text:
FLORES 2023 use a number of 13 TeV Run 2 searches at the LHC to place constraints on the  compactification scale 1/R and cutoff scale Lambda in the minimal universal extra  dimension model  with Standard Model fields propagating in the bulk (see their Fig.6).


pdgid: S071KK
text:
AVNISH 2021 perform a study on the ATLAS collaboration search for multiple jets plus missing transverse energy from p p collisions at sqrt(s) = 13 TeV and integrated luminosity of 139 fb**-1, to place constraints on the compactification scale and cutoff scale Lambda in universal extra dimension models with Standard Model fields propagating in the bulk.


pdgid: S071KK
text:
AABOUD 2018AV use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV in final states with multiple b-jets, to place a lower bound on the compactification scale in a model with two universal extra dimensions. Assuming the radii of the two extra dimensions are equal, a lower limit of 1.8 TeV for the Kaluza-Klein mass is obtained.


pdgid: S071KK
text:
AABOUD 2018CE use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV in final states with same-charge leptons and b-jets, to place a lower bound on the compactification scale in a model with two universal extra dimensions. Assuming the radii of the two extra dimensions are equal, a lower limit of 1.45 TeV for the Kaluza-Klein mass is obtained.


pdgid: S071KK
text:
ACCOMANDO 2015 use electroweak precision observables to place a lower bound on the compactification scale 1/R. See their Fig. 2 for the bound as a function of  sin(beta), which parametrizes the VEV contribution from brane and bulk Higgs fields. The  quoted value is for the minimum bound which occurs at sin(beta) = 0.45.


pdgid: S071KK
text:
KHACHATRYAN 2015T use 19.7 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV to place a lower bound on the compactification scale 1/R.


pdgid: S071KK
text:
CHATRCHYAN 2013AQ use 5.0 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV and a further 3.7 fb**-1 of data at sqrt(s) = 8 TeV to place a lower bound on the compactification scale 1/R, in models with universal extra dimensions and Standard Model fields propagating in the bulk. See their Fig. 5 for the bound as a function of the universal bulk fermion mass parameter mu.


pdgid: S071KK
text:
CHATRCHYAN 2013W use diphoton events with large missing transverse momentum in 4.93 fb**-1 of data produced from p p collisions at sqrt(s) = 7 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M_{{c}} = 20. The model parameters are chosen such that the decay gamma^* --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
EDELHAUSER 2013 use 19.6 and 20.6 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV analyzed by the CMS Collaboration in the dielectron and dimuon channels, respectively, to place a lower bound on the mass of the second lightest Kaluza-Klein Z/gamma boson (converted to a limit on 1/R = M_{{c}}). The bound assumes Standard Model fields propagating in the bulk and that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M_{{c}} = 20.


pdgid: S071KK
text:
AAD 2012CP use diphoton events with large missing transverse momentum in 4.8 fb**-1 of data produced from p p collisions at sqrt(s) = 7 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M_{{c}} = 20. The model parameters are chosen such that the decay gamma^* --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
AAD 2012X use diphoton events with large missing transverse momentum in 1.07 fb**-1 of data produced from p p collisions at sqrt(s) = 7 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M_{{c}} = 20. The model parameters are chosen such that the decay gamma^* --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
ABAZOV 2012M use same-sign dimuon events in 7.3 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the compactification scale 1/R, in models with universal extra dimensions where all Standard Model fields propagate in the bulk.


pdgid: S071KK
text:
BAAK 2012 use electroweak precision observables to place a lower bound on the compactification scale 1/R, in models with universal extra dimensions and Standard Model fields propagating in the bulk. Bound assumes a 125 GeV Higgs mass. See their Fig. 25 for the bound as a function of the Higgs mass.


pdgid: S071KK
text:
FLACKE 2012 use electroweak precision observables to place a lower bound on the compactification scale 1/R, in models with universal extra dimensions and Standard Model fields propagating in the bulk. See their Fig. 1 for the bound as a function of the universal bulk fermion mass parameter mu.


pdgid: S071KK
text:
NISHIWAKI 2012 use up to 2 fb**-1 of data from the ATLAS and CMS experiments that constrains the production cross section of a Higgs-like particle to place a lower bound on the compactification scale 1/R in universal extra dimension models. The quoted bound assumes Standard Model fields propagating in the bulk and a 125 GeV Higgs mass. See their Fig. 1 for the bound as a function of the Higgs mass.


pdgid: S071KK
text:
AAD 2011F use diphoton events with large missing transverse energy in 3.1 pb**-1 of data produced from p p collisions at sqrt(s) = 7 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M(c) = 20. The model parameters are chosen such that the decay gamma^*() --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
AAD 2011X use diphoton events with large missing transverse energy in 36 pb**-1 of data produced from p p collisions at sqrt(s) = 7 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M_{{c}} = 20. The model parameters are chosen such that the decay gamma^*() --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
ABAZOV 2010P use diphoton events with large missing transverse energy in 6.3 fb**-1 of data produced from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the compactification scale in a universal extra dimension model with gravitational decays. The bound assumes that the cutoff scale Lambda, for the radiative corrections to the Kaluza-Klein masses, satisfies Lambda/M(c)=20. The model parameters are chosen such that the decay gamma^*() --> G gamma occurs with an appreciable branching fraction.


pdgid: S071KK
text:
ABAZOV 2009AE use dijet angular distributions in 0.7 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the compactification scale.


pdgid: S071KK
text:
HAISCH 2007 use inclusive Bbar-meson decays to place a Higgs mass independent bound on the compactification scale 1/R in the minimal universal extra dimension model.


pdgid: S071KK
text:
GOGOLADZE 2006 use electroweak precision observables to place a lower bound on the compactification scale in models with universal extra dimensions. Bound assumes a 115 GeV Higgs mass. See their Fig. 3 for the bound as a function of the Higgs mass.


pdgid: S071KK
text:
CORNET 2000 translates a bound on the coefficient of the 4-fermion operator (leptonbar gamma_mu tau^a lepton)(leptonbar gamma^mu tau^a lepton) derived by Hagiwara and Matsumoto into a limit on the mass scale of KK W bosons.


pdgid: S071KK
text:
RIZZO 2000 obtains limits from global electroweak fits in models with a Higgs in the bulk (3.8 TeV) or on the standard brane (3.3 TeV).


pdgid: S071RSG
text:
SIRUNYAN 2021N use 137 (140) fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for dilepton resonances in the dielectron (dimuon) channel. See Table 6 for other limits with warp parameter values k/Mbar_{{P}} = 0.01 and 0.05. This updates the results of SIRUNYAN 2018BB.


pdgid: S071RSG
text:
HAYRAPETYAN 2024AE use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar W W final state. See their Figure 19 for limits on the cross section times branching fraction as a function of the KK graviton mass for k/Mbar_{{P}} = 0.3, 0.5 and 1.


pdgid: S071RSG
text:
HAYRAPETYAN 2024AJ use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV, in the diphoton channel to place a lower limit on the mass of the lightest KK graviton. See their paper for limits with other warp parameter values k/Mbar_{{P}} = 0.01 and 0.2. This updates the results of SIRUNYAN 2018DU.


pdgid: S071RSG
text:
TUMASYAN 2024B use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the gamma gamma b bbar final state. See their Figure 6 for limits on the cross section times branching fraction as a function of the KK graviton mass assuming k/Mbar_{{P}} = 0.5 and 1. This updates the result of SIRUNYAN 2019.


pdgid: S071RSG
text:
TUMASYAN 2023AP use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for W W, Z Z diboson resonances in q qbar q qbar final states. See their Figure 7 for the limit on the cross section times branching fraction as a function of the KK graviton mass. Assuming k/Mbar_{{P}} = 0.5, a graviton mass is excluded below 1400 GeV. This updates the result of SIRUNYAN 2020Q.


pdgid: S071RSG
text:
AAD 2022F use 126 -- 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar b bbar final state. See their Figure 14 for limits on the cross section times branching fraction as a function of the KK graviton mass. Assuming k/Mbar_{{P}} = 1, gravitons in the mass range 298 -- 1460 GeV are excluded. This updates the results of AABOUD 2019A.


pdgid: S071RSG
text:
TUMASYAN 2022D use 137 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for W W resonances in lepton nu q q final states (lepton = e, mu). See their Figure 6 for the limit on the KK graviton mass as a function of the cross section times branching fraction, including theoretical values for k/Mbar_{{P}} = 0.5. This updates the results of SIRUNYAN 2018AX.


pdgid: S071RSG
text:
TUMASYAN 2022J use 137 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Z Z resonances in the nu nubar q qbar final state. See their Figure 10 for the limit on the KK graviton mass as a function of the cross section times branching fraction, assuming k/Mbar_{{P}} = 0.5. This updates the result of SIRUNYAN 2018BK.


pdgid: S071RSG
text:
TUMASYAN 2022R use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Z Z resonances in 2 lepton 2 q final states (lepton = e, mu). See their Figure 8 for the limit on the KK graviton mass as a function of the cross section times branching fraction. Assuming k/Mbar_{{P}} = 0.5, a graviton mass is excluded below 1200 GeV. This updates the result of SIRUNYAN 2018DJ.


pdgid: S071RSG
text:
TUMASYAN 2022U use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to  search for Higgs boson pair production in the b bbar q qbar^' lepton nu, b bbar lepton nu lepton nu  and b bbar lepton nu nu lepton nu nu final states (lepton = e, mu). See their  Figure 7 for limits on the cross section times branching fraction as a function of the KK graviton  mass, including theoretical values for k/Mbar_{{P}} = 0.3 and 0.5. This updates the  results of SIRUNYAN 2019CF and SIRUNYAN 2018F.


pdgid: S071RSG
text:
AAD 2021AF use 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Z Z resonances in the lepton lepton lepton lepton and lepton lepton nu nubar final states (lepton=e, mu). See their Figure 8 for the limit on the cross section times branching fraction as a function of the KK graviton mass, including theoretical values for k/Mbar_{{P}} = 1. This updates the results of AAD 2015AU and AABOUD 2018BF.


pdgid: S071RSG
text:
AAD 2021AY use 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV in the diphoton channel to place a lower limit on the mass of the lightest KK graviton. This updates the results of AABOUD 2017AP.


pdgid: S071RSG
text:
AAD 2020AT use 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for diboson resonances in semileptonic final states (lepton nu q q,lepton lepton q q, nu nu q q). See their Figure 15 for the limit on the cross section times branching fraction as a function of the KK graviton mass. Lower limits on the graviton mass are also given for k/Mbar_{{P}} = 1. This updates the results of AABOUD 2018AK and AABOUD 2018AL.


pdgid: S071RSG
text:
AAD 2020C use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar b bbar, b bbar W+ W-, and b bbar tau+ tau- final states. See their Figure 5(b)(c) for limits on the cross section as a function of the KK graviton mass. In the case of k/Mbar_{{P}} = 1 and 2, gravitons are excluded in the mass range 260 -- 3000 GeV and 260 -- 1760 GeV, respectively.


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AAD 2020T use 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for narrow resonances decaying to bottom quark pairs. See their Figure 7 for the limit on the product of the cross section, branching fraction, acceptance and b-tagging efficiency as a function of the KK graviton mass. In the case of k/Mbar_{{P}} = 0.2, KK gravitons in the mass range 1.25 -- 2.8 TeV are excluded.


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SIRUNYAN 2020AI use 137 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for dijet resonances. See their Figure 6 for the limit on the product of the cross section, branching fraction and acceptance as a function of the KK graviton mass. This updates the results of SIRUNYAN 2018BO.


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SIRUNYAN 2020F use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar Z Z final state. See their Figure 4 for limits on the cross section times branching fraction as a function of the KK graviton mass, and Figure 5 for limits as a function of k/Mbar_{{P}}.


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AABOUD 2019O use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar W W final state. See their Figure 12 for limits on the cross section times branching fraction as a function of the KK graviton mass for k/Mbar_{{P}} = 1 and k/Mbar_{{P}} = 2.


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AAD 2019D use 139 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for diboson resonances in the all-hadronic final state. See their Figure 9(b) for the limit on the cross section times branching fraction as a function of the KK graviton mass, including theoretical values for k/Mbar_{{P}} = 1. This updates the results of AABOUD 2018F.


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SIRUNYAN 2019BE use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production by combining the results from four final states: b bbar gamma gamma, b bbar tau taubar, b bbar b bbar, and b bbar V V. See their Figure 7 for limits on the cross section times branching fraction as a function of the KK graviton mass.


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AABOUD 2018BI use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for top-quark pairs decaying into the lepton-plus jets topology. See their Figure 16 for the limit on the KK graviton mass as a function of the cross section times branching fraction, including theoretical values for k/Mbar_{{P}} = 1.


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AABOUD 2018CJ combine the searches for heavy resonances decaying into bosonic and leptonic final states from 36.1 fb**-1 of p p collision data at sqrt(s) = 13 TeV. The lower limit on the KK graviton mass, with k/Mbar_{{P}} = 1, is 2.3 TeV.


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AABOUD 2018CQ use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar tau+ tau- final state. See their Figure 2 for limits on the cross section times branching fraction as a function of the KK graviton mass. Assuming k/Mbar_{{P}} = 1, gravitons in the mass range 325 -- 885 GeV are excluded.


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AABOUD 2018CW use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the gamma gamma b bbar final state. See their Figure 7 for limits on the cross section times branching fraction as a function of the KK graviton mass.


pdgid: S071RSG
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SIRUNYAN 2018AF use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar b bbar final state. See their Figure 9 for limits on the cross section times branching fraction as a function of the KK graviton mass, including theoretical values for k/Mbar_{{P}} = 0.5. This updates the results of KHACHATRYAN 2015R.


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SIRUNYAN 2018AS use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Z Z resonances in the lepton lepton nu nubar final state (lepton=e, mu). See their Figure 5 for the limit on the KK graviton mass as a function of the cross section times branching fraction, including theoretical values for k/Mbar_{{P}} = 0.1, 0.5, and 1.0.


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SIRUNYAN 2018CW use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for Higgs boson pair production in the b bbar b bbar final state. See their Figure 8 for limits on the cross section times branching fraction as a function of the KK graviton mass, including theoretical values for k/Mbar_{{P}} = 0.5.


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SIRUNYAN 2018I use 19.7 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV to search for narrow resonances decaying to bottom quark pairs. See their Figure 3 for the limit on the KK graviton mass as a function of the cross section times branching fraction in the mass range of 325 -- 1200 GeV.


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AAD 2016R use 20.3 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV to place a lower bound on the mass of the lightest KK graviton. See their Figure 4 for the limit on the KK graviton mass as a function of the cross section times branching fraction.


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AAD 2015AZ use 20.3 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV to place a lower bound on the mass of the lightest KK graviton. See their Figure 2 for limits on the KK graviton mass as a function of the cross section times branching ratio.


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AAD 2015CP use 20.3 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV to place a lower bound on the mass of the lightest KK graviton. See their Figures 6b and 6c for the limit on the KK graviton mass as a function of the cross section times branching fraction.


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AAD 2014V use 20.3 (20.5) fb**-1 of data from p p collisions at sqrt(s) = 8 TeV in the dielectron (dimuon) channels to place a lower bound on the mass of the lightest KK graviton. This updates the results of AAD 2012CC.


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AAD 2013A use 4.7 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV in the lepton nu lepton nu channel, to place a lower bound on the mass of the lightest KK graviton.


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AAD 2013AO use 4.7 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV in the lepton nu j j channel, to place a lower bound on the mass of the lightest KK graviton.


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AAD 2013AS use 4.9 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV in the diphoton channel to place lower limits on the mass of the lightest KK graviton. The diphoton channel is combined with previous results in the dielectron and dimuon channels to set the best limit. See their Table 2 for warp parameter values k/Mbar_{{P}} between 0.01 and 0.1. This updates the results of AAD 2012Y.


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AAD 2012AD use 1.02 fb**-1 of data from p p collisions at sqrt(s) = 7 TeV to search for KK gravitons in a warped extra dimension decaying to Z Z dibosons in the l l j j and l l l l channels (lepton=e, mu). The limit is quoted for the combined l l j j + l l l l channels. See their Figure 5 for limits on the cross section CS(G --> Z Z) as a function of the graviton mass.


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AALTONEN 2012V use 6 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in a warped extra dimension decaying to Z Z dibosons in the l l j j and l l l l channels (lepton=e, mu). It provides improved limits over the previous analysis in AALTONEN 2011G. See their Figure 16 for limits from all channels combined on the cross section times branching ratio CS(p pbar --> G^* --> Z Z) as a function of the graviton mass.


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BAAK 2012 use electroweak precision observables to place a lower bound on the compactification scale k e**-pi k R, assuming Standard Model fields propagate in the bulk and the Higgs is confined to the IR brane. See their Fig. 27 for more details.


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AALTONEN 2011G use 2.5 -- 2.9 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in a warped extra dimension decaying to Z Z dibosons via the e e e e, e e mu mu, mu mu mu mu, e e j j, and mu mu j j channels. See their Fig. 20 for limits on the cross section CS(G --> Z Z) as a function of the graviton mass.


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AALTONEN 2011R uses 5.7 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV in the dielectron channel to place a lower bound on the mass of the lightest graviton. It provides combined limits with the diphoton channel analysis of AALTONEN 2011U. For warp parameter values k/Mbar_{{P}} between 0.01 to 0.1 the lower limit on the mass of the lightest graviton is between 612 and 1058 GeV. See their Table I for more details.


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ABAZOV 2011H use 5.4 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the mass of the lightest graviton. Their 95% C.L. exclusion limit does not include masses less than 300 GeV.


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AALTONEN 2010N use 2.9 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the mass of the lightest graviton.


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ABAZOV 2010F use 5.4 fb**-1 of data from p pbar collisions at sqrt(s) = 1.96 TeV to place a lower bound on the mass of the lightest graviton. For warp parameter values of k/Mbar_{{P}} between 0.01 and 0.1 the lower limit on the mass of the lightest graviton is between 560 and 1050 GeV. See their Fig. 3 for more details.


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AALTONEN 2008S use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to four electrons via two Z bosons using 1.1 fb**-1 of data. See their Fig. 8 for limits on sigma.B(G --> Z Z) versus the graviton mass.


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ABAZOV 2008J use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to electrons and photons using 1 fb**-1 of data. For warp parameter values of k/Mbar_{{P}} between 0.01 and 0.1 the lower limit on the mass of the lightest excitation is between 300 and 900 GeV. See their Fig. 4 for more details.


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AALTONEN 2007G use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to photons using 1.2 fb**-1 of data. For warp parameter values of k/Mbar_{{P}} = 0.1, 0.05, and 0.01 the bounds on the graviton mass are 850, 694, and 230 GeV, respectively. See their Fig. 3 for more details. See also AALTONEN 2007H.


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AALTONEN 2007H use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to electrons using 1.3 fb**-1 of data. For a warp parameter value of k/Mbar_{{P}} = 0.1 the bound on the graviton mass is 807 GeV. See their Fig. 4 for more details. A combined analysis with the diphoton data of AALTONEN 2007G yields for k/Mbar_{{P}} = 0.1 a graviton mass lower bound of 889 GeV.


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ABAZOV 2005N use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to muons, electrons or photons, using 260~pb**-1 of data. For warp parameter values of k/Mbar_{{P}} = 0.1, 0.05, and 0.01, the bounds on the graviton mass are 785, 650 and 250 GeV respectively. See their Fig. 3 for more details.


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ABULENCIA 2005A use p pbar collisions at sqrt(s) = 1.96 TeV to search for KK gravitons in warped extra dimensions. They search for graviton resonances decaying to muons or electrons, using 200~pb**-1 of data. For warp parameter values of k/Mbar_{{P}} = 0.1, 0.05, and 0.01, the bounds on the graviton mass are 710, 510 and 170 GeV respectively.


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AABOUD 2018BI use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV. This result updates AAD 2013AQ.


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HAYRAPETYAN 2024G use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to place limits on a KK gluon decaying to gluons via a spin-0 radion, R. See their Figure 3 for limits on the cross section times branching fraction as a function of the KK gluon mass and various values of the radion mass. This updates the results of TUMASYAN 2022C.


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AABOUD 2019AS use 36.1 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV. An upper bound of 3.4 TeV is placed on the KK gluon mass for Gamma/m = 30%.


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SIRUNYAN 2019AL use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to place limits on a KK gluon decaying to a top quark and a heavy vector-like fermion, T. KK gluon masses between 1.5 and 2.3 TeV and between 2.0 and 2.4 TeV are excluded for T masses of 1.2 and 1.5 TeV, respectively.


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CHATRCHYAN 2013BM use 19.7 fb**-1 of data from p p collisions at sqrt(s) = 8 TeV. Bound is for a width of approximately 15 -- 20% of the KK gluon mass.


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CHEN 2013A place limits on the KK mass scale for a specific warped model with custodial symmetry and bulk fermions. See their Figures 4 and 5.


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SIRUNYAN 2018DA use 35.9 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for semiclassical black holes decaying to multijet final states. No excess of events above the expected level of standard model background was observed. Exclusions at 95% CL are set on the mass threshold for black hole production as a function of the higher-dimensional Planck scale for rotating and nonrotating black holes under several model assumptions (ADD, 2, 4, 6 extra dimensions model) in the 7.1 -- 10.3 TeV range. These limits supersede those in SIRUNYAN 2017CP.


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AAD 2016N use 3.6 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for semiclassical black hole decays to multijet final states. No excess of events above the expected level of Standard Model background was observed. Exclusion contours at 95% C.L. are set on the mass threshold for black hole production versus higher-dimensional Planck scale for rotating black holes (ADD, 6 extra dimensions model).


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AAD 2016O use 3.2 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for semiclassical black hole decays to high-mass final states with leptons and jets. No excess of events above the expected level of Standard Model background was observed. Exclusion contours at 95% C.L. are set on the mass threshold for black hole production versus higher-dimensional Planck scale for rotating black holes (ADD, 2 to 6 extra dimensions).


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AAD 2013AW use 20.3 fb^{-1} of data from p p collisions at sqrt(s) = 8 TeV to search for semiclassical black hole decays to like-sign dimuon final states using large track multiplicity. No excess of events above the expected level of Standard Model background was observed. Exclusion contours at 95% C.L. are set on the mass threshold for black hole production versus higher-dimensional Planck scale in various extra dimensions, rotating and non-rotating models.


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AAD 2024S use 140 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays to final states with high-invariant-mass lepton + jet. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in an ADD (6 extra dimensions) model and the Randall-Sundrum (one extra dimension) model. The resulting lower mass threshold limits in the ADD (RS) models are 9.2 (6.8) TeV. The ADD limit supersedes that in AAD 2014AL.


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AAD 2023CB use 139 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays with different-flavor high-mass dilepton final states. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in ADD (6 extra dimensions) and RS1 models. Assuming the black hole mass threshold is equal to the higher-dimensional Planck scale, mass thresholds below 5.9 (3.8), 5.2 (3.0), and 5.1 (3.0) TeV are excluded in the e mu, e tau and mu tau channels for the ADD (RS1) models, respectively. These limits supersede those in AABOUD 2018CM.


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TUMASYAN 2023AW use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays in the tau lepton plus missing transverse momentum final state. Assuming the black hole mass threshold is equal to the higher-dimensional Planck scale, threshold masses below 6.6 TeV are excluded in the ADD model with four extra dimensions (see their Figure 8).


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TUMASYAN 2023BC use 138 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays to final states with a photon and a jet. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in ADD (6 extra dimensions) and RS1 models. Assuming the black hole mass threshold is equal to the higher-dimensional Planck scale, mass thresholds below 7.5 TeV and 5.2 TeV are excluded for the ADD and RS1 models, respectively (see their Figure 9).


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TUMASYAN 2023H use 138 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to  search for quantum black hole decays with different-flavor high-mass dilepton final states. No  excess of events above the expected level of Standard Model background was observed. Exclusion  limits at 95% C.L. are set on mass thresholds for black hole production in the ADD model (with 4 extra dimensions). Assuming the black hole mass threshold is equal to the higher-dimensional  Planck scale, mass thresholds below 5.6, 5.2, and 5.0 TeV are excluded in the e mu, e tau  and mu tau channels, respectively.


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AAD 2020T use 139 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays to final states with dijets. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in an ADD (6 extra dimensions) model. Assuming the black hole mass threshold is equal to the higher-dimensional Planck scale, mass thresholds below 9.4 TeV are excluded. This limit supersedes AABOUD 2017AK.


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AABOUD 2018BA use 36.7 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays to final states with a photon and a jet. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in ADD (6 extra dimensions) and RS1 models. Assuming the black hole mass threshold is equal to the Planck scale, mass thresholds below 7.1 TeV and 4.4 TeV are excluded for the ADD and RS1 models, respectively. These limits supersede those in AAD 2016AI.


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SIRUNYAN 2018AT use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays to e mu final states. In Figure 4, lower mass limits of 5.3, 5.5 and 5.6 TeV are placed in a model with 4, 5 and 6 extra dimensions, respectively, and a lower mass limit of 3.6 TeV is found for a single warped dimension.


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SIRUNYAN 2018DD use 35.9 fb**-1 of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black hole decays in dijet angular distributions. A lower mass limit of 5.9 (8.2) TeV is placed in the RS (ADD) model with one (six) extra dimension(s).


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SIRUNYAN 2017CP use 2.3 fb^{-1} of data from p p collisions at sqrt(s) = 13 TeV to search for quantum black holes decaying to dijet final states. No excess of events above the expected level of standard model background was observed. Limits on the quantum black hole mass threshold are set as a function of the higher-dimensional Planck scale, under the assumption that the mass threshold must exceed the above Planck scale. Depending on the model, mass thresholds in the range up to 5.1 -- 9.0 TeV are excluded.


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KHACHATRYAN 2016BE use 19.7 fb^{-1} of data from p p collisions at sqrt(s) = 8 TeV to search for quantum black holes undergoing lepton flavor violating decay to the e mu final state. No excess of events above the expected level of standard model background was observed. Exclusion limits at 95% CL are set on mass thresholds for black hole production in the ADD (2 -- 6 flat extra dimensions), RS1 (1 warped extra dimension), and a model with a Planck scale at the TeV scale from a renormalization of the gravitational constant (no extra dimensions). Limits on the black hole mass threshold are set assuming that it is equal to the higher-dimensional Planck scale. Mass thresholds for quantum black holes in the range up to 3.15 -- 3.63 TeV are excluded in the ADD model. In the RS1 model, mass thresholds below 2.81 TeV are excluded in the PDG convention for the Schwarzschild radius. In the model with no extra dimensions, mass thresholds below 1.99 TeV are excluded.


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KHACHATRYAN 2015V use 19.7 fb^{-1} of data from p p collisions at sqrt(s) = 8 TeV to search for quantum black holes decaying to dijet final states. No excess of events above the expected level of standard model background was observed. Exclusion limits at 95% CL are set on mass thresholds for black hole production in the ADD (2 -- 6 flat extra dimensions) and RS1 (1 warped extra dimension) model. Limits on the black hole mass threshold are set as a function of the higher-dimensional Planck scale, under the assumption that the mass threshold must exceed the above Planck scale. Depending on the model, mass thresholds in the range up to 5.0 -- 6.3 TeV are excluded. This paper supersedes CHATRCHYAN 2013AD.


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AAD 2014V use 20.3 (20.5) fb^{-1} of data in the dielectron (dimuon) channels from p p collisions at sqrt(s) = 8 TeV to search for quantum black hole decays involving high-mass dilepton resonances. No excess of events above the expected level of Standard Model background was observed. Exclusion limits at 95% C.L. are set on mass thresholds for black hole production in ADD (6 extra dimensions) and RS1 models. Assuming the black hole mass threshold is equal to the higher-dimensional Planck scale, mass thresholds below 3.65 TeV and 2.24 TeV are excluded for the ADD and RS1 models, respectively.


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CHATRCHYAN 2013A use 5 fb^{-1} of data from p p collisions at sqrt(s) = 7 TeV to search for quantum black holes decaying to dijet final states. No excess of events above the expected level of standard model background was observed. Exclusion limits at 95% CL are set on mass thresholds for black hole production in the ADD (2 -- 6 flat extra dimensions) and RS (1 warped extra dimension) model. Limits on the black hole mass threshold are set as a function of the higher-dimensional Planck scale, under assumption that the mass threshold must exceed the above Planck scale. Depending on the model, mass thresholds in the range up to 4.0 -- 5.3 TeV are excluded.


pdgid: S030DI5
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ANGLOHER 2024 search for spin-independent light WIMP (mass between 0.16 and 6 GeV) scatter on diamond target. No signal observed. Limits placed in sigma^SI vs mass plane for sub-GeV WIMPs. Quoted limit is for m(WIMP) = 0.2 GeV.


pdgid: S030DI5
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ANGLOHER 2024B search for low mass m(wimp) ~100 MeV. No signal observed. Limits placed in cross section vs. mass plane. Quoted limit for m(wimp) = 100 MeV.


pdgid: S030DI5
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AALBERS 2023A search for e recoil events from GeV scale WIMP scatter on Xe. No signal observed. Limits placed on 6 different models including sigma^SI < 3E-3 for m(chi) ~ 1 GeV via Migdal scattering.


pdgid: S030DI5
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AGNES 2023 for for light DM via e recoil/Migdal effect. No signal observed. sigma^SI(chiN) < 4E-7 pb for m(chi) = 3 GeV.


pdgid: S030DI5
text:
AGNES 2023B search for GeV-scale DM scatter on nucleons in Ar. No signal observed. Limit sigma^SI(chi N) < 6E-7 pb for m(chi) = 3 GeV.


pdgid: S030DI5
text:
ALBAKRY 2023 search for light DM via Migdal effect. No signal observed. Allow sigma^SI < 0.5 pb for m(chi)=1 GeV (see e.g. Fig. 7).


pdgid: S030DI5
text:
AMBROSONE 2023 derive limits on sigma(chi p) due to possible DM distortion of cosmic ray spectra in starburst galaxies. Limits placed in sigma vs. mass (E-3 -- 10 MeV) plane, the most stringent given above being at 1 keV.


pdgid: S030DI5
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ANGLOHER 2023 search for light DM using Si target. No signal observed. Require sigma^SI < 70 pb for m(chi) = 0.3 GeV (see e.g. Fig. 5).


pdgid: S030DI5
text:
LI 2023F searches for SI light DM scatter from Xe. No signal observed. The quoted limit for m(chi) = 4 GeV.


pdgid: S030DI5
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MA 2023A search for GeV-scale DM using PandaX-4T. No signal observed. sigma(chi p) < 5E-10 pb for m(chi) = 10 GeV.


pdgid: S030DI5
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ADHIKARI 2022B search for sub-GeV WIMPs via SI and SD detection; no signal detected; limits placed in m(chi) vs. sigma plane for m(chi): 0.2 -- 3 GeV; quoted limit is for m(chi) = 1 GeV.


pdgid: S030DI5
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ARMENGAUD 2022 search for GeV-scale DM scatter on Ge at EDELWEISS via Migdal  effect; no signal observed; limits placed in sigma^SI(chi N) vs. m(DM) plane; quoted limit  is for m(DM) = 100 MeV.


pdgid: S030DI5
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CUI 2022 search for sub-GeV boosted DM at PandaX-II at CJPL; no signal detected; limits set in sigma^SI(chi p) vs. m(chi) plane; quoted limit for m(chi) = 0.1 GeV.


pdgid: S030DI5
text:
XU 2022 search for sub-GeV boosted DM in CDEX; no signal observed; limits placed in CS(chi N) vs. m(DM) plane; quoted limit is for m(DM) = 0.1 GeV.


pdgid: S030DI5
text:
AKERIB 2021A present new technique for low mass WIMP detection. Require sigma^SI(p chi) < 2E-7 pb for m(WIMP) 10 GeV.


pdgid: S030DI5
text:
ALKHATIB 2021 search for light DM using SuperCDMS; require sigma^SI(p chi) < 5E6 for m(DM) = 0.1 GeV.


pdgid: S030DI5
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ANDRIAMIRADO 2021A search for upscattered (boosted) sub-GeV DM interacting with proton in PROSPECT detector. No signal observed. Limits placed in sigma(chi N) vs. m(DM) plane for m(DM) ~ 1  keV - 0.5 GeV. The listed limit is for m(DM) = 1 keV.


pdgid: S030DI5
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APRILE 2021 search for low recoil energy GeV-scale DM in XENON1T with 1.6 keV threshold. No signal in 0.6 t y exposure. Limits placed in sigma^SI(chi N) vs. m(DM) plane for m(DM) between 3 -- 12 GeV. The listed limit is for m(DM) = 5 GeV.


pdgid: S030DI5
text:
AGUILAR-AREVALO 2020C search for WIMP SI scatter on Si using DAMIC at SNOLab; some excess; limits placed in sigma vs m(DM) for m(DM) in 1.2 -- 10 GeV; quoted limit for m(WIMP) = 2 GeV.


pdgid: S030DI5
text:
AKERIB 2020A search for GeV-scale WIMPs via WIMP-nucleon scatter with single photon emission; no signal; limits placed in m(WIMP) vs sigma^SI plane: for example sigma^SI(chi n) < 8E-4 pb for m(WIMP) = 2.5 GeV.


pdgid: S030DI5
text:
ABDELHAMEED 2019A search for GeV scale dark matter SI scatter on CaWO(4); no signal, limits placed in sigma vs. mass plane for m(DM) ~ 0.1 -- 10 GeV. The listed limit is for m(DM) = 1 GeV.


pdgid: S030DI5
text:
AGNESE 2019A search for 1.5 -- 10 GeV WIMP scatter on Ge in CDMSlite dataset. Limits set in a likelihood analysis. No signal was observed. Limit reported for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AKERIB 2019 search for 0.4 -- 5 GeV DM using bremsstrahlung photons and "Migdal" electrons; 1.4E4 kg d exposure of liquid Xe; constraint sigma^SI(chi N) < 1 pb for m(chi) = 5 GeV in light scalar mediator model.


pdgid: S030DI5
text:
AMOLE 2019 search for SI WIMP scatter on C(3)F(8) in PICO-60 bubble chamber; no signal: set limit for spin independent coupling sigma^SI(chi N) < 1E-6 pb for m(chi) = 5 GeV.


pdgid: S030DI5
text:
APRILE 2019C search for light DM scatter on Xe via atomic excitation, ionization (Migdal effect) or bremsstrahlung; no signal, limits placed in sigma vs. m(DM) plane for m(DM) ~ 0.085 -- 2 GeV. The listed limit is for m(DM) = 1 GeV.


pdgid: S030DI5
text:
APRILE 2019D search for light DM scatter on Xe via ionization to probe SI, SD, and chi e cross sections; with 22 t d exposure, limits placed in various sigma vs. m(DM) planes. Quoted limit is for m(DM) = 5 GeV.


pdgid: S030DI5
text:
ARMENGAUD 2019search for GeV scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 0.045 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
KOBAYASHI 2019 search for sub-GeV WIMP annual modulation in Xe via brems; no signal; limits placed in sigma^SI(chi N) vs. m(chi) plane for m ~ 0.3 -- 1 GeV; quoted limit is for m(chi) = 0.5 GeV.


pdgid: S030DI5
text:
LIU 2019B seach for sub-GeV DM using Migdal effect on Ge at CDEX-IB; no signal, require sigma^SI(chi N) < 7E2 pb for m(chi) = 0.1 GeV.


pdgid: S030DI5
text:
AGNESE 2018 search for GeV scale WIMPs using CDMSlite; limits placed in sigma^SI(chi N) vs. m(chi) plane for m ~ 1.5 -- 20 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
APRILE 2018 search for WIMP scatter on 1 t yr Xe; no signal, limits set in sigma(chi N) vs. m(chi) plane for m(chi) ~ 6 -- 1000 GeV; quoted limit is for m = 6 GeV.


pdgid: S030DI5
text:
ARNAUD 2018 search for low mass WIMP scatter on Ne via SPC at NEWS-G; limits set in sigma^SI(chi N) vs. m(chi) plane for m ~ 0.5 -- 20 GeV; quoted limit is for m = 5 GeV.


pdgid: S030DI5
text:
JIANG 2018 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 3 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
YANG 2018 search for WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 2 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AKERIB 2017 search for WIMP scatter on Xe; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
ANGLOHER 2017A search for GeV scale WIMP scatter on Al(2)O(3) crystal; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 0.15 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
ANGLOHER 2016 search for GeV scale WIMP scatter on CaWO(4); limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 0.5 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
APRILE 2016 search for low mass WIMPs via ionization at XENON100; limits placed in sigma**SI(chi N) vs m(chi) plane for m ~ 3.5 -- 20 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
ARMENGAUD 2016 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
HEHN 2016 search for low mass WIMPs via SI scatter on Ge target using profile likelihood analysis; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
ZHAO 2016 search for GeV-scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AMOLE 2015 search for WIMP scatter on C(3)F(8) in PICO-2L; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 25 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
XIAO 2015 search for WIMP scatter on Xe with PandaX-I; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 100 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AGNESE 2014 search for GeV scale WIMPs SI scatter at SuperCDMS; no signal, limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 3.5 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AKERIB 2014 search for WIMP scatter on Xe; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 5000 GeV. Limit given for m(chi) = 5 GeV.


pdgid: S030DI5
text:
LI 2013B search for WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 100 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
ARCHAMBAULT 2012 search for low mass WIMP scatter on C(4)F(10); limits set in sigma^SI(chi N) vs. m(chi) plane for m ~ 4 -- 12 GeV; quoted limit is for m = 5 GeV.


pdgid: S030DI5
text:
AALSETH 2011 search for GeV-scale SI WIMP scatter on Ge; limits placed on sigma**SI(chi N) for m(chi) ~ 3.5 -- 100 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AHMED 2011B search for GeV scale WIMP scatter on Ge in CDMS II; limits placed in sigma^SD(chi n) vs. m(chi) plane for m ~ 4 -- 12 GeV.


pdgid: S030DI5
text:
ANGLE 2011 search for GeV scale WIMPs in Xenon-10; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 20 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DI5
text:
AKERIB 2010 search for WIMP scatter on Ge/Si in CDMS II; limits place in sigma_{{SI}}(chi N) vs. m(chi) plane for m ~ 3 -- 100 GeV. Limit given for m(DM) = 5 GeV.


pdgid: S030DI1
text:
ANGLOHER 2024A search for WIMP scatter on NaI target. No signal observed. Limits placed in sigma^SI vs m plane.


pdgid: S030DI1
text:
AALBERS 2023 present first limits for WIMP scatter on Xe. sigma^SI(chi p) < 1E-11 pb for m(chi) = 20 GeV.


pdgid: S030DI1
text:
ABE 2023E search for WIMP scatter on Xe in XMASS. No signal observed. Require sigma^SI < 2E-7 pb for m(chi) = 20 GeV.


pdgid: S030DI1
text:
APRILE 2023A present first results from Xe-nton SI WIMP search. No signal observed. Quoted limit is for m(chi) = 20 GeV.


pdgid: S030DI1
text:
MENG 2021B search for SI WIMP interaction with 3.7 t Xe and 0.63 t yr exposure. No signal observed. Limits placed in m(DM) vs. sigma**SI plane.


pdgid: S030DI1
text:
ANGLOHER 2019 search for low mass WIMP scatter on CaWO(4); no signal; limits placed on Wilson coefficients for m(chi) = 0.6 -- 60 GeV.


pdgid: S030DI1
text:
KIM 2019A search for WIMP scatter in NaI KIMS experiment; no signal: require sigma^SI(chi n) < 7E-5 pb for m(chi) = 20 GeV.


pdgid: S030DI1
text:
KOBAYASHI 2019 search for WIMP scatter in XMASS single-phase liquid Xe detector; no signal; require sigma^SI(chi N) < 3E-7 pb for m(chi) = 20 GeV.


pdgid: S030DI1
text:
SEONG 2019 search for Upsilon --> gamma A, A --> chi chi via CP-odd Higgs; no signal; limits on BF set; model dependent conversion to WIMP-nucleon scattering cross section limits sigma**SI < E-36 cm**2 for m(chi) = 0.01 -- 1 GeV.


pdgid: S030DI1
text:
YANG 2019 search for low mass wimps via annual modulation in Ge; no signal; require sigma^SI(chi N) < 3.5E-5 pb for m(chi) = 20 GeV.


pdgid: S030DI1
text:
ABE 2018C search for WIMP annual modulation signal for m(WIMP): 6 -- 20 GeV; limits set on SI WIMP-nucleon cross section: see Fig. 6.


pdgid: S030DI1
text:
ADHIKARI 2018 search for WIMP scatter on NaI; no signal; require sigma**SI < 1.44E-5 pb for m(WIMP) = 20 GeV; inconsistent with DAMA/LIBRA result.


pdgid: S030DI1
text:
AGNES 2018 search low mass m(WIMP): 1.8 -- 20 GeV scatter on Ar; limits on SI WIMP-nucleon cross section set in Fig. 8.


pdgid: S030DI1
text:
AGNESE 2018 give limits for sigma^SI(chi N) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.


pdgid: S030DI1
text:
AGNESE 2018A search for WIMP scatter on Ge at SuperCDMS; 1 event, consistent with expected background; set limit in sigma^SI(chi N) vs. m(chi) plane for m ~ 10 -- 250 GeV.


pdgid: S030DI1
text:
APRILE 2018 search for WIMP scatter on 1 t yr Xe; no signal, limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 6 -- 1000 GeV.


pdgid: S030DI1
text:
ARNAUD 2018 search for low mass WIMP scatter on Ne via SPC at NEWS-G; limits set in sigma^SI(chi N) vs. m(chi) plane for m ~ 0.5 -- 20 GeV.


pdgid: S030DI1
text:
AKERIB 2017 search for WIMP scatter on Xe; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV.


pdgid: S030DI1
text:
BARBOSA-DE-SOUZA 2017 search for annual modulation of WIMP scatter on NaI using an exposure of 61 kg yr of DM-Ice17 for recoil energy in the 4 -- 20 keV range (DAMA found modulation for recoil energy < 5 keV). No modulation seen. Sensitivity insufficient to distinguish DAMA signal from null.


pdgid: S030DI1
text:
CUI 2017A search for SI WIMP scatter; limits placed in sigma^SI(chi N) vs. m(chi) plane for m ~ 10 -- 1E4 GeV using 54 ton-day exposure of Xe.


pdgid: S030DI1
text:
AGNESE 2016 CDMSlite excludes low mass WIMPs 1.6 -- 5.5 GeV and SI scattering cross section depending on m(WIMP); see Fig. 4.


pdgid: S030DI1
text:
ANGLOHER 2016 search for GeV scale WIMP scatter on CaWO(4); limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 0.5 -- 30 GeV.


pdgid: S030DI1
text:
APRILE 2016 search for low mass WIMPs via ionization at XENON100; limits placed in sigma**SI(chi N) vs m(chi) plane for m ~ 3.5 -- 20 GeV.


pdgid: S030DI1
text:
ARMENGAUD 2016 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV.


pdgid: S030DI1
text:
HEHN 2016 search for low mass WIMPs via SI scatter on Ge target using profile likelihood analysis; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV.


pdgid: S030DI1
text:
ZHAO 2016 search for GeV-scale WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV.


pdgid: S030DI1
text:
AGNESE 2015A reanalyse AHMED 2011B low threshold data. See their Fig. 12 (left) for  improved limits extending down to 5 GeV.


pdgid: S030DI1
text:
XIAO 2015 search for WIMP scatter on Xe with PandaX-I; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 100 GeV.


pdgid: S030DI1
text:
This limit value is provided by the authors. See their Fig. 4 for limits extending down to mass(X0) = 3.5 GeV.


pdgid: S030DI1
text:
This limit value is provided by the authors. AGNESE 2014A result is from CDMSlite mode operation with enhanced sensitivity to low mass mass(X0). See their Fig. 3 for limits extending down to mass(X0) = 3.5 GeV (see also Fig. 4 in AGNESE 2014).


pdgid: S030DI1
text:
LIU 2014A result is based on prototype CDEX-0 detector. See their Fig. 13 for limits extending down to mass(X0) = 2 GeV.


pdgid: S030DI1
text:
AARTSEN 2013 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the sun in data taken between June 2010 and May 2011.


pdgid: S030DI1
text:
This limit value is provided by the authors. AGNESE 2013 use data taken between Oct. 2006 and July 2007. See their Fig. 4 for limits extending down to mass(X0) = 7 GeV.


pdgid: S030DI1
text:
This limit value is provided by the authors. AGNESE 2013A use data taken between July 2007 and Sep. 2008. Three candidate events are seen. Assuming these events are real, the best fit parameters are mass(X0) = 8.6 GeV and sigma = 1.9E-5 pb.


pdgid: S030DI1
text:
This limit value is provided by the authors. Limit from combined data of AGNESE 2013 and AGNESE 2013A. See their Fig. 4 for limits extending down to mass(X0) = 5.5 GeV.


pdgid: S030DI1
text:
BERNABEI 2013A search for annual modulation of counting rate in the 2 -- 6 keV recoil energy interval, in a 14 yr live time exposure of 1.33 t yr. Find a modulation of 0.0112+-0.0012 counts/(day kg keV) with 9.3 sigma C.L. Find period and phase in agreement with expectations from DM particles.


pdgid: S030DI1
text:
LI 2013B search for WIMP scatter on Ge; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 4 -- 100 GeV.


pdgid: S030DI1
text:
ANGLOHER 2012 observe excess events above the expected background which are consistent with X0 with mass ~ 25 GeV (or 12 GeV) and spin-independent X0-nucleon cross section of 2E-6 pb (or 4E-5 pb).


pdgid: S030DI1
text:
AALSETH 2011A find indications of annual modulation of the data, the energy spectrum being compatible with X0 mass around 8 GeV. See also AALSETH 2013.


pdgid: S030DI1
text:
AHMED 2011 search for X0 inelastic scattering. See their Fig. 8 -- 10 for limits. The inelastic cross section reduces to the elastic cross section at the limit of zero mass splitting (Fig. 8, left).


pdgid: S030DI1
text:
APRILE 2011A search for X0 inelastic scattering. See their Fig. 2 and 3 for limits. See also APRILE 2014A.


pdgid: S030DI2
text:
AALBERS 2023 present first LZ limits on SI WIMP-nucleon scatter from Xe. sigma^SI(chi p) < 2.5E-11 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
ABE 2023E search for WIMP scatter on Xe in XMASS. No signal observed. Require sigma^SI < 2E-7 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
APRILE 2023A present first results from Xe-nton SI WIMP search. No signal observed. Quoted limit is for m(chi) = 100 GeV.


pdgid: S030DI2
text:
ADHIKARI 2020 search for SI WIMP scatter from Ar in AJAJ 2019 data. No signal observed. Limits placed on sigma^p vs. m(WIMP) for various assumed operators and models.


pdgid: S030DI2
text:
ABE 2019 search for SI DD in single phase Xe; no signal; require sigma^SI(chi p) < 4E-8 pb for m(chi) ~ 100 GeV.


pdgid: S030DI2
text:
AJAJ 2019 search for SI WIMP-nucleon scatter with 758 tonne day exposure of single phase liquid Ar; no signal: require sigma^SI(chi N) < 3.9E-9 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
ADHIKARI 2018 search for WIMP scatter on NaI;limit set sigma**SI(chi p) < 2.3E-6 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
AGNES 2018A search for WIMP scatter on 46.4 kg Ar; no signal; require sigma^SI(chi N) < 1.14E-8 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
AMAUDRUZ 2018 search for WIMP scatter on Ar with DEAP-3600; limits set: sigma**SI(chip) < 1.2E-8 pb for m(WIMP) = 100 GeV.


pdgid: S030DI2
text:
APRILE 2018 search for WIMP scatter on 1.3 t liquid Xe; no signal; require sigma^SI(chi p) < 9.12E-11 pb for m(chi) = 100 GeV.


pdgid: S030DI2
text:
REN 2018 search for self-interacting DM at Panda-X-II with a total exposure of 54 ton day; limits set in m(DM) vs. m(mediator) plane.


pdgid: S030DI2
text:
AKERIB 2017 exclude SI cross section > 1.7E-10 pb for m(WIMP) = 100 GeV. Uses complete LUX data set.


pdgid: S030DI2
text:
APRILE 2017G set limit sigma**SI(chi p) < 1.2 E-10 pb for m(WIMP) = 100 GeV using 1 ton fiducial mass Xe TPC. Exposure is 34.2 live days.


pdgid: S030DI2
text:
AKERIB 2016 re-analysis of 2013 data exclude SI cross section > 1E-9 pb for m(WIMP) = 100 GeV on Xe target.


pdgid: S030DI2
text:
APRILE 2016B combined 447 live days using Xe target exclude sigma(SI) > 1.1E-9 pb for m(WIMP) = 50 GeV.


pdgid: S030DI2
text:
AVRORIN 2014 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the Sun in data taken between 1998 and 2003. See their Table 1 for limits assuming annihilation into neutrino pairs.


pdgid: S030DI2
text:
ADRIAN-MARTINEZ 2013 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the sun in data taken between Jan. 2007 and Dec. 2008.


pdgid: S030DI2
text:
BOLIEV 2013 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the sun in data taken from 1978 to 2009. See also SUVOROVA 2013 for an older analysis of the same data.


pdgid: S030DI2
text:
ABBASI 2012 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the Sun. The amount of X0 depends on the X0-proton cross section.


pdgid: S030DI2
text:
AJELLO 2011 search for e+- flux from X0 annihilations in the Sun. Models in which X0 annihilates into an intermediate long-lived weakly interacting particles or X0 scatters inelastically are constrained. See their Fig. 6 -- 8 for limits.


pdgid: S030DI2
text:
GIULIANI 2005 analyzes the spin-independent X0-nucleon cross section limits with both isoscalar and isovector couplings. See their Fig. 3 and 4 for limits on the couplings.


pdgid: S030DI3
text:
AALBERS 2023 give first LZ limits on WIMP-nucleon scatter from Xe. sigma^SI < 2.8E-10 pb for m(chi) = 1 TeV.


pdgid: S030DI3
text:
ABE 2023E search for WIMP scatter on Xe in XMASS. No signal observed. Require sigma^SI < 2E-7 pb for m(chi) = 1000 GeV.


pdgid: S030DI3
text:
ADHIKARI 2020 search for SI WIMP scatter from Ar in AJAJ 2019 data. No  signal observed. Limits placed on sigma^p vs. m(WIMP) for various assumed operators and models.


pdgid: S030DI3
text:
YAGUNA 2019 recasts DEAP-3600 single-phase liquid argon results in limit for isospin violating DM; for f_{{n}}/f_{{p}} = -0.69, requires sigma^SI(chi p) < 3E-6  pb for m(chi) = 1 TeV.


pdgid: S030DI3
text:
AGNES 2018A search for WIMP scatter on 46.4 kg Ar; no signal; require sigma^SI(chi N) < 3.8E-8 pb for m(chi) = 1 TeV.


pdgid: S030DI3
text:
APRILE 2018 search for WIMP scatter on 1.3 t Xe; no signal seen; require sigma^SI(chi p) < 8.24E-10 pb for m(chi) = 1 TeV.


pdgid: S030DI3
text:
AKERIB 2017 search for WIMP scatter on Xe using complete LUX data set; limits placed in sigma^SI(chi N) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV.


pdgid: S030DI3
text:
CHEN 2017E search for inelastic WIMP scatter on Xe; require sigma**SI(chi N) < 0.3 pb for m(chi) = 1 TeV and (mass difference) = 300 keV.


pdgid: S030DI3
text:
CUI 2017A search for WIMP scatter using 54 ton-day exposure of Xe; limits placed in sigma^SI(chi N) vs. m(chi) plane for m ~ 10 -- 1E4 GeV.


pdgid: S030DI6
text:
AALBERS 2024A search for ultraheavy dark matter in range 10E8 -- 10E17 GeV via multiple scatter. No signal observed. Limits placed in sigma^SI vs m plane for two different nuclear scaling possibilities.


pdgid: S030DI6
text:
ABREU 2023 search for superheavy DM X decay to q qbar pairs via instanton, then  to gammas. No signal detected. Exclude m(X) > 3E13 GeV for dark gauge coupling  alpha_{{X}} = 0.09.


pdgid: S030DI6
text:
ACEVEDO 2023 re-examine data from ancient mica to place limits on superheavy DM in the mass range E7 -- E25 GeV. See Fig. 3 for sigma^SI and sigma^SD limits.


pdgid: S030DP5
text:
ANGLOHER 2024B search for low mass wimps. No signal observed. Limits placed in sigma vs. m plane. Quoted limit for m = 100 MeV.


pdgid: S030DP5
text:
AALBERS 2023A search for GeV-scale WIMP scatter on Xe. No signal observed. Limits placed in sigma^SD(chi p) vs. m(chi) plane. Quoted limit is for m(chi) = 1 GeV via Migdal scattering.


pdgid: S030DP5
text:
ADHIKARI 2022B search for sub-GeV WIMPs via SI and SD detection; no signal detected; limits  placed in m(chi) vs. sigma plane for m(chi): 0.2 -- 3 GeV; quoted limit is for SD m(chi) = 1 GeV.


pdgid: S030DP5
text:
ANGLOHER 2022 search for SD WIMP-proton scatter from Li target; no signal detected; limits placed in sigma vs. m(WIMP) plane; limit quoted for m(WIMP) = 1 GeV.


pdgid: S030DP5
text:
ANGLOHER 2022A search for spin-dependent DM scatter on Li and Al for m(DM) ~  0.2 -- 6 GeV; no signal observed; limits set in CS(chi p) vs. m(DM) plane; quoted  limit is for m(DM) = 1 GeV.


pdgid: S030DP5
text:
ABDELHAMEED 2020A use LiAlO(2) target in CRESST to search for SD WIMP scatter on p; no signal; quoted limit is for m(DM) = 1 GeV.


pdgid: S030DP5
text:
ABDELHAMEED 2019 search for SD WIMP scatter on Li7; limits placed on sigma^SD(chi p) for m(chi) ~ 0.8 -- 20 GeV; quoted limit is for m(chi) = 1 GeV.


pdgid: S030DP5
text:
AMOLE 2019 search for SD WIMP scatter on C(3)F(8) in PICO-60 bubble chamber; no signal: set limit for spin dependent coupling sigma^SD(chi p) < 2E-4 pb for m(chi) = 5 GeV.


pdgid: S030DP5
text:
APRILE 2019C search for light DM on Xe via Migdal/brem effect; no signal, require sigma^SD(chi p) < 1.7E4 pb for m(chi) = 1 GeV.


pdgid: S030DP5
text:
ARMENGAUD 2019 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 0.5 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP5
text:
XIA 2019A search for WIMP scatter on Xe in PandaX-II; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP5
text:
AGNESE 2018 search for GeV scale WIMPs with CDMSlite; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 1.5 -- 20 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP5
text:
AKERIB 2017A search for SD WIMP scatter on Xe using 129.5 kg yr exposure; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 6 -- 1E5 GeV.


pdgid: S030DP5
text:
FU 2017 search for SD WIMP scatter on Xe; limits set in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 4 -- 1E3 GeV.; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP5
text:
AMOLE 2015 search for WIMP scatter on C(3)F(8) in PICO-2L; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 4 -- 1E4 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP5
text:
ARCHAMBAULT 2012 search for SD WIMP scatter in F19 with PICASSO; limits set in sigma^SD(chi p) vs. m(chi) plane for m ~ 4 -- 500 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DP1
text:
AALBERS 2023 yield first SD LZ limits on WIMP-p scatter using Xe. sigma^SD(chi p) < 6E-5 pb for m(chi) = 20 GeV.


pdgid: S030DP1
text:
ABBASI 2022B search for WIMP annihilation to b bbar, tau taubar, nu nubar in Sun with 7 years data; no signal; limits set in m(chi) vs. sigma^SD(chi p) plane for m(chi): 10 -- 100 GeV; quoted limit for nu nubar channel.


pdgid: S030DP1
text:
ANGLOHER 2022 search for SD WIMP-proton scatter from Li target; no signal detected; limits placed in sigma vs. m(WIMP) plane.


pdgid: S030DP1
text:
HUANG 2022 search for SD DM scatter on Xe; no signal observed; limits placed in CS(chi n) vs. m(DM) plane; quoted limit is for m(DM) = 20 GeV.


pdgid: S030DP1
text:
AARTSEN 2020C place combined IceCube and Pico-60 velocity-independent limits on spin-dependent WIMP-p scatter sigma^SD(chi p)< 9 -- 5 pb for m(WIMP) = 20 GeV assuming dominant annihilation to tau taubar.


pdgid: S030DP1
text:
ABDELHAMEED 2020A use LiAlO(2) target in CRESST to search for spin-dependent WIMP scatter on p; limits set for m(WIMP): 0.3 -- 30 GeV in Fig. 8. Quoted limit is for M(WIMP) = 30 GeV.


pdgid: S030DP1
text:
ABDELHAMEED 2019 uses Li(2)MoO(4) target to set limit for spin dependent coupling sigma^SD(chi p) < 3.E5 pb for m(chi) = 20 GeV.


pdgid: S030DP1
text:
AMOLE 2019 search for SD WIMP scatter on C(3)F(8) in PICO-60 bubble chamber; no signal: set limit for spin dependent coupling sigma^SD(chi p) < 2.5E-5 pb for m(chi) = 20 GeV.


pdgid: S030DP1
text:
APRILE 2019A search for SD WIMP scatter on 1 t yr Xe; no signal, limits placed in sigma^SD(chi p) vs. m(chi) plane for m ~ 6 -- 1000 GeV.


pdgid: S030DP1
text:
XIA 2019A search for WIMP scatter on Xe in PandaX-II; limits placed in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV.


pdgid: S030DP1
text:
AGNESE 2018 give limits for sigma^SD(p chi) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.


pdgid: S030DP1
text:
BEHNKE 2017 show final Picasso results based on 231.4 kg d exposure at SNOLab for WIMP scatter on C(4)F(10) search via superheated droplet; require sigma(SD) < 1.32E-2 pb for m(WIMP) = 20 GeV.


pdgid: S030DP1
text:
FU 2017 search for SD WIMP scatter on Xe; limits set in sigma^SD(chi p) vs. m(chi) plane for m(chi) ~ 4 -- 1E3 GeV.


pdgid: S030DP1
text:
AMOLE 2016A require SD WIMP-p scattering < 5E-4 pb for m(WIMP) = 20 GeV; bubbles from C(3)F(8) target.


pdgid: S030DP1
text:
KHACHATRYAN 2016AJ require SD WIMP-p < 2E-6 pb for m(WIMP) = 20 GeV from p p --> Z + notET; Z --> lepton leptonbar signal.


pdgid: S030DP1
text:
The value has been provided by the authors. APRILE 2013 note that the proton limits on Xe are highly sensitive to the theoretical model used. See also APRILE 2014A.


pdgid: S030DP1
text:
ARCHAMBAULT 2012 search for WIMP scatter on C(4)F(10); limits set in sigma^SD(chi p) vs. m(chi) plane for m ~ 4 -- 500 GeV.


pdgid: S030DP1
text:
TANAKA 2011 search for neutrinos from the Sun arising from the pair annihilation of X0 trapped by the Sun. The amount of X0 depends on the X0-proton cross section.


pdgid: S030DP2
text:
AALBERS 2023 yield first SD LZ limits on WIMP-p scatter using Xe. sigma^SD(chi p) < 1.5E-4 pb for m(chi) = 100 GeV.


pdgid: S030DP2
text:
ADHIKARI 2023C search for SD WIMP scatter on I. No signal observed. Require sigma^SD(chi p) < 1 pb for m(chi) = 100 GeV.


pdgid: S030DP2
text:
SHIMADA 2023 search for WIMPs in NEWAGE directional detector. No signal observed. Limits placed in sigma^SD(chi p) vs. mass plane. Quoted limit for m(chi) = 150 GeV.


pdgid: S030DP2
text:
HUANG 2022 search for SD DM scatter on Xe; no signal observed; limits placed in CS(chi n) vs. m(DM) plane; quoted limit is for m(DM) = 100 GeV.


pdgid: S030DP2
text:
IKEDA 2021 use direction sensitive TPC NEWAGE to search for SD WIMPs. No signal observed. Limits set in sigma^SD(chi p) vs. m plane; sigma^SD(chi p) < 50 pb for m(DM) = 100 GeV.


pdgid: S030DP2
text:
AARTSEN 2020C place combined IceCube and Pico-60 velocity-independent limits on spin-dependent WIMP-p scatter sigma^SD(chi p) < 3.34E-4 pb for m(WIMP) = 100 GeV assuming dominant annihilation to tau taubar.


pdgid: S030DP2
text:
AMOLE 2019 search for SD WIMP scatter on C(3)F(8) in PICO-60 bubble chamber; no signal: set limit for spin dependent coupling sigma^SD(chi p) < 4E-5 pb for m(chi) = 100 GeV.


pdgid: S030DP2
text:
AMOLE 2017 require CS(WIMP-p)**SD < 5E-5 pb for m(WIMP) = 100 GeV using PICO-60 1167 kg-days exposure at SNOLab.


pdgid: S030DP2
text:
APRILE 2017A require require CS(WIMP-p)(inelastic)**SD < 3.3E-2 pb for m(WIMP) = 100 GeV, based on 7640 kg day exposure at LNGS.


pdgid: S030DP2
text:
BATTAT 2017 use directional detection of CS(2) ions to require CS(SD) < 2.8E-1 pb for 100 GeV WIMP with a 55 days exposure at the Boulby Underground Science Facility.


pdgid: S030DP2
text:
FU 2017 from a 33000 kg d exposure at CJPL, PANDAX II derive for m(DM) = 100 GeV, sigma^SD(WIMP-p) <2E-3 pb.


pdgid: S030DP2
text:
AABOUD 2016D use ATLAS 13 TeV 3.2 fb^{-1} of data to search for monojet plus missing E(T); agree with SM rates; present limits on large extra dimensions, compressed SUSY spectra and wimp pair production.


pdgid: S030DP2
text:
AABOUD 2016F search for monophoton plus missing E(T) events at ATLAS with 13 Tev and 3.2 fb**-1; signal agrees with SM background; place limits on SD WIMP-proton scattering vs. mediator mass and large extra dimension models.


pdgid: S030DP2
text:
AARTSEN 2016C search for high energy nus from WIMP annihilation in solar core; limits set on SD WIMP-p scattering (Fig. 8).


pdgid: S030DP2
text:
ADRIAN-MARTINEZ 2016 search for WIMP annihilation into nus from solar core; exclude SD cross section < few E-4 depending on m(WIMP).


pdgid: S030DP2
text:
AMOLE 2016 use bubble technique on CF(3)I target to exclude SD WIMP-p scattering > 5E-4 pb for m(WIMP) = 100 GeV.


pdgid: S030DP3
text:
AALBERS 2023 yield first SD LZ limits on WIMP-p scatter using Xe. sigma^SD(chi p) < 2E-3 pb for m(chi) = 1 TeV.


pdgid: S030DP3
text:
ADHIKARI 2023C search for SD WIMP scatter on I. No signal observed. Require sigma^SD(chi p) < 0.2 pb for m(chi) = 1 TeV.


pdgid: S030DP3
text:
HUANG 2022 search for SD DM scatter on Xe; no signal observed; limits placed in CS(chi n) vs. m(DM) plane; quoted limit is for m(DM) = 1 TeV.


pdgid: S030DP3
text:
IKEDA 2021 use direction sensitive TPC NEWAGE to search for SD WIMPs. No signal observed. Limits set in sigma^SD(chi p) vs. m plane; sigma^SD(chi p) < 200 pb for m(DM) = 1000 GeV.


pdgid: S030DP3
text:
AARTSEN 2020C place combined IceCube and Pico-60 velocity-independent limits on spin-dependent WIMP-p scatter sigma^SD(chi p) < 3E-3 pb for m(WIMP) = 1 TeV assuming dominant annihilation to W W.


pdgid: S030DP3
text:
AMOLE 2019 search for SD WIMP scatter on C(3)F(8) in PICO-60 bubble chamber; no signal: set limit for spin dependent coupling sigma^SD(chi p) < 3E-4 pb for m(chi) = 1000 GeV.


pdgid: S030DP3
text:
ALBERT 2018C search for DM annihilation in Sun to long-lived mediator (LLM) which decays outside Sun, for DM masses above 1 TeV; assuming LLM, limits set on sigma**SD(chi p).


pdgid: S030DP3
text:
AARTSEN 2017A search for neutrinos from solar WIMP annihilation into tau+ tau- in 532 days of live time.


pdgid: S030DP3
text:
ADRIAN-MARTINEZ 2016B search for secluded DM via WIMP annihilation in solar core into light mediator which later decays to mu or nus; limits presented in Figures 3 and 4.


pdgid: S030DN5
text:
AALBERS 2023A search for GeV-scale WIMP scatter on Xe. No signal observed. Limits placed in sigma^SD(chi n) vs. m(chi) plane. Quoted limit is for m(chi) = 1 GeV via Migdal scattering.


pdgid: S030DN5
text:
ANGLOHER 2022 search for SD WIMP scatter on Li target; no signal detected; limits placed on WIMP-neutron SD scatter versus m(WIMP); limit quoted for m(WIMP) = 1 GeV.


pdgid: S030DN5
text:
ANGLOHER 2022A search for spin-dependent DM scatter on Li and Al for m(DM) ~  0.2 -- 6 GeV; no signal observed; limits set in CS(chi n) vs. m(DM) plane; quoted  limit is for m(DM) = 1 GeV.


pdgid: S030DN5
text:
ABDELHAMEED 2020A use LiAlO(2) target in CRESST to search for SD WIMP scatter; no signal; quoted limit is for m(DM) = 1 GeV.


pdgid: S030DN5
text:
ABDELHAMEED 2019 search for GeV-scale WIMP SD scatter on Li7 crystal; set limit sigma^SD(chi n) for m(chi) ~ 0.8 -- 20 GeV; quoted limit for m(chi) = 1 GeV.


pdgid: S030DN5
text:
APRILE 2019C search for light DM on Xe via Migdal/bremsstrahlung effect; no signal, require sigma^SD(chi n) <230 pb for m(chi) = 1 GeV.


pdgid: S030DN5
text:
APRILE 2019D search for light DM scatter on Xe via ionization; no signal, limits placed in sigma vs. m(DM) ~ 3 -- 6 GeV; quoted limit is for m(DM) = 5 GeV.


pdgid: S030DN5
text:
ARMENGAUD 2019 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 0.5 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
XIA 2019A search for WIMP scatter on Xe in PandaX-II; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
AGNESE 2018 search for GeV scale WIMPs scatter at CDMSlite; limits placed in sigma^SD(chi n) vs. m(chi) plane for m ~ 1.5 -- 20 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
JIANG 2018 search for GeV scale WIMP scatter on Ge; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 3 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
YANG 2018 search for WIMP scatter on Ge; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 2 -- 10 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
AKERIB 2017A search for SD WIMP scatter on Xe with 129.5 kg yr exposure; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
FU 2017 search for SD WIMP scatter on Xe; limits set in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 4 -- 1E3 GeV.; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
ZHAO 2016 search for GeV-scale WIMP scatter on Ge; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV; quoted limit is for m(chi) = 5 GeV.


pdgid: S030DN5
text:
AHMED 2011B search for GeV scale WIMP scatter on Ge in CDMS II; limits placed in sigma^SD(chi n) vs. m(chi) plane for m ~ 4 -- 12 GeV. Limit given for m(chi) = 5 GeV.


pdgid: S030DN1
text:
AALBERS 2023 yield first LZ limits on SD WIMP-n scatter using Xe.  sigma^SD(chi n)< 2E-6 pb for m(chi) = 20 GeV.


pdgid: S030DN1
text:
ANGLOHER 2022 search for SD WIMP-neutron scatter from Li target; no signal detected; limits placed in sigma vs. m(WIMP) plane.


pdgid: S030DN1
text:
ABDELHAMEED 2020A use LiAlO(2) target in CRESST to search for SD WIMP scatter on n; limits placed for m(WIMP): 0.3 -- 30 GeV in Fig. 8. Quoted limit is for M(WIMP) = 30 GeV.


pdgid: S030DN1
text:
APRILE 2019A search for SD WIMP scatter on 1 t yr Xe; no signal: limits placed in sigma^SD(chi n) vs. m(chi) plane for m ~ 6 -- 1000 GeV.


pdgid: S030DN1
text:
XIA 2019A search for WIMP scatter on Xe in PandaX-II; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV.


pdgid: S030DN1
text:
AGNESE 2018 give limits for sigma^SD(n chi) for m(WIMP) between 1.5 and 20 GeV using CDMSlite mode data.


pdgid: S030DN1
text:
AKERIB 2017A search for SD WIMP scatter on Xe with 129.5 kg yr exposure; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 5 -- 1E5 GeV.


pdgid: S030DN1
text:
FU 2017 search for SD WIMP scatter on Xe; limits set in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 4 -- 1E3 GeV.


pdgid: S030DN1
text:
ZHAO 2016 search for GeV-scale WIMP scatter on Ge; limits placed in sigma^SD(chi n) vs. m(chi) plane for m(chi) ~ 4 -- 30 GeV.


pdgid: S030DN2
text:
AALBERS 2023 yield first LZ limits on SD WIMP-n scatter using Xe. sigma(chi n) < 5E-6 pb for m(chi) = 100 GeV.


pdgid: S030DN2
text:
APRILE 2019A search for SD WIMP scatter on 1 t yr Xe; no signal, limits placed in sigma^SD(chi n) vs. m(chi) plane for m ~ 6 -- 1000 GeV.


pdgid: S030DN2
text:
SUZUKI 2019 search in single phase liquid xenon detector for inelastic scattering X0 + ^129Xe --> X0 + ^129Xe* (39.58 keV) ; no signal: require CS(chi n)**SD < 4E-3 pb for m(chi) = 100 GeV.


pdgid: S030DN2
text:
UCHIDA 2014 derived limit from search for inelastic scattering X0 + ^129Xe --> X0 + ^129Xe(39.58 keV).


pdgid: S030DN2
text:
MIUCHI 2003 give model-independent limit for spin-dependent X0-proton and neutron cross sections. See their Fig. 5.


pdgid: S030DN3
text:
AALBERS 2023 yield first LZ SD limits on WIMP-n scatter on Xe. sigma^SD(chi n) < 5E-5 pb for m(chi) = 1 TeV.


pdgid: S030DE5
text:
SHANG 2024 report on search for electron cosmic-ray boosted DM in keV range or below with PandaX-4T. No signal observed. Limits plotted in sigma(chi e) vs m plane for m ~E-2 -- E3 keV.


pdgid: S030DE5
text:
ZHANG 2024A examine detection of accelerated MeV-scale DM on e in Ge semiconductor. Limits placed in sigma_{{e}} vs. m plane depending on various mediator assumptions.


pdgid: S030DE5
text:
AGNES 2023A search for MeV-scale DM scatter from e using Ar. No signal observed. sigma(chi e) < 3E-3 pb for m(chi) = 30 MeV.


pdgid: S030DE5
text:
ARNQUIST 2023A search for LDM scatter on e using CCDs. No signal observed. Require  sigma(chi e) < 0.3 pb for m(chi) = 10 MeV and F(DM) = 1 (Fig. 3b).


pdgid: S030DE5
text:
LI 2023F search for light DM in MeV range via scatter from e. No signal observed. Limits set. The quoted limit is for m(chi) = 0.2 GeV with F(DM) = 1.


pdgid: S030DE5
text:
AGOSTINI 2022 search for superWIMP particles using GERDA detector; no signal observed; limits placed in mass vs coupling plane for m(DM) 0.06 -- 1 MeV.


pdgid: S030DE5
text:
APRILE 2022 place new limits on WIMP-e scatter for dark photon and various multipole moments vs. WIMP mass for various DM models; quoted limit for m(WIMP) = 1 GeV in light mediator model.


pdgid: S030DE5
text:
BATTAGLIERI 2022 search for light MeV scale DM particles produced in JLAB beam dump; no  signal observed; limits set in kinetic mixing vs. m(DM) plane for m(DM) ~ 1 -- 200 MeV.


pdgid: S030DE5
text:
BOSE 2022 theoretically derive limits on WIMP-e scatter from solar gamma rays using data of Fermi-LAT; limit quoted for m(WIMP) = 5 GeV.


pdgid: S030DE5
text:
GHOSH 2022 derive limits on sub-GeV boosted DM scatter from e or nu using  SuperK/XENON1T data; quoted limit for m(chi) = 1 MeV.


pdgid: S030DE5
text:
HOCHBERG 2022 search for sub-eV or sub-MeV scale DM scatter/absorption on e in superconducting nanowire; no signal observed; limits set in m(DM) vs. cross section plane for sub-MeV-scale DM and in m(DM) vs. kinetic mixing plane for sub-eV-scale DM.


pdgid: S030DE5
text:
ZHANG 2022A search for DM scatter on e using CDEX-10; no signal observed; limits placed on CS(chi e) vs. m(DM) plane for m(DM) ~ 0.07 -- 10 GeV for various simplified models.


pdgid: S030DE5
text:
CHENG 2021 search for MeV-scale DM scatter from e in PANDAX-II. No signal detected. Limits set in sigma(chi e) vs. m(DM) plane for two choices of form factors; sigma(chi e) < 10 pb for m(chi) = 10 MeV and F(DM) = 1.


pdgid: S030DE5
text:
AKERIB 2020 search for mirror DM with LUX 95 d x 118 kg data for mirror e scatter from Xe; no signal, limits placed in kinetic mixing parameter vs. mirror e temperature T ~ 0.1 -- 0.9 keV plane.


pdgid: S030DE5
text:
AMARAL 2020 search SuperCDMS data for low mass DM scatter from e in Si; no signal; quoted limit sigma_{{e}} < 8.7E2 pb for m(DM) = 10 MeV with form factor F(DM) = 1.


pdgid: S030DE5
text:
APRILE 2020 report excess at electron recoil around 2 -- 3 keV in Xe; data compared to unforeseen tritium background, and various signal models (bosonic DM, solar axion, and neutrino magnetic moment).


pdgid: S030DE5
text:
ARNAUD 2020 search for MeV DM scattering from e in Ge; no signal; quoted limit is for m(DM) = 10 MeV with form factor F(DM) = 1.


pdgid: S030DE5
text:
BARAK 2020 report search for MeV scale DM scatter from e in Si; limits placed in sigma_{{e}} vs. m(DM) plane; quoted limit is for m(DM) = 10 MeV and form factor F(DM) = 1.


pdgid: S030DE5
text:
ABRAMOFF 2019 search for MeV-scale WIMP scatter from Si skipper-CCD; limits placed on sigma(chi e) for m(chi) ~ 0.5 -- 100 MeV depending on DM form factors. Limit given for m(DM) = 1 MeV.


pdgid: S030DE5
text:
AGUILAR-AREVALO 2019A search for MeV scale DM scatter from e in Si CCDs at SNOLAB; no signal, limits placed in CS(e) vs. m(DM) plane for m(DM) ~ 0.6 -- 100 MeV.


pdgid: S030DE5
text:
APRILE 2019D search for light DM scatter on Xe via ionization; no signal, limits placed in sigma on nucleus vs. m(DM) plane for m(DM) ~ 0.02 -- 10 GeV; quoted limit is for m(DM) = 0.2 GeV.


pdgid: S030DE5
text:
AGNES 2018B search for MeV scale WIMP scatter from e in Ar; no signal, limits set in sigma_{{e}} vs. m(chi) plane for m ~ 20 -- 1000 MeV and two choices of form factor F(DM); quoted limit for m(chi) = 100 MeV and F = 1.


pdgid: S030DE5
text:
AGNESE 2018B search for e chi scatter in SuperCDMS; limits placed in sigma(e chi) vs. m(chi) plane for m ~ 0.3 -- 1E4 MeV for two assumed form factors and also in m(dark photon) vs. kinetic mixing plane. Limit given for m(chi) = 1 GeV and F=1.


pdgid: S030DE5
text:
CRISLER 2018 search for chi e --> chi e scatter in Si CCD; place limits on MeV DM in sigma_{{e}} vs. m(chi) plane for m ~ 0.5 -- 1000 MeV for different form factors; quoted limit is for F(DM) = 1 and m(chi) = 10 MeV.


pdgid: S030DE5
text:
APRILE 2017 search for WIMP-e annual modulation signal for recoil energy in the 2.0 -- 5.8 keV interval using 4 years data with Xe. No significant effect seen.


pdgid: S030DM5
text:
AKIMOV 2022 use COHERENT CsI(Na) detector to search for sub GeV DM particles produced by the  Spallation Neutron Source; no signal observed; limits placed in mediator mass vs. coupling plane  for leptophobic DM models.


pdgid: S030DM1
text:
BENOIT 2000 find four event categories in Ge detectors and suggest that low-energy surface nuclear recoils can explain anomalous events reported by UKDMC and Saclay NaI experiments.


pdgid: S030DM1
text:
BELLI 1996C use background subtraction and obtain sigma<150 pb (<1.5 fb) (90% CL) for spin-dependent (independent) X0-proton cross section. The confidence level is from R. Bernabei, private communication, May 20, 1999.


pdgid: S030DM1
text:
BERNABEI 1996 use pulse shape discrimination to enhance the possible signal. The limit here is from R. Bernabei, private communication, September 19, 1997.


pdgid: S030DM1
text:
SARSA 1996 search for annual modulation of WIMP signal. See SARSA 1997 for details of the analysis. The limit here is from M.L. Sarsa, private communication, May 26, 1997.


pdgid: S030DM1
text:
SMITH 1996 use pulse shape discrimination to enhance the possible signal. A dark matter density of 0.4 GeV cm**-3 is assumed.


pdgid: S030DM1
text:
GARCIA 1995 limit is from the event rate. A weaker limit is obtained from searches for diurnal and annual modulation.


pdgid: S030DM1
text:
SNOWDEN-IFFT 1995 look for recoil tracks in an ancient mica crystal. Similar limits are also given for Al27 and Si28. See COLLAR 1996 and SNOWDEN-IFFT 1996 for discussion on potential backgrounds.


pdgid: S030DM1
text:
REUSSER 1991 limit here is changed from published (0.04) after reanalysis by authors. J.L. Vuilleumier, private communication, March 29, 1996.


pdgid: S030DM2
text:
APRILE 2021A search for inelastic DM scatter off Xe129 nuclei with 0.83 t yr  exposure. No signal obseved. Limits placed in sigma(chiXe) vs. m(DM) plane for WIMP mass between 20 GeV and 10 TeV.


pdgid: S030DM2
text:
BELLI 2002 discuss dependence of the extracted WIMP cross section on the assumptions of the galactic halo structure.


pdgid: S030DM2
text:
BERNABEI 2002C analyze the DAMA data in the scenario in which X0 scatters into a slightly heavier state as discussed by SMITH 2001.


pdgid: S030DM2
text:
GREEN 2002 discusses dependence of extracted WIMP cross section limits on the assumptions of the galactic halo structure.


pdgid: S030DM2
text:
ULLIO 2001 disfavor the possibility that the BERNABEI 1999 signal is due to spin-dependent WIMP coupling.


pdgid: S030DM2
text:
AMBROSIO 1999 search for upgoing muon events induced by neutrinos originating from WIMP annihilations in the Sun and Earth.


pdgid: S030DM2
text:
BRHLIK 1999 discuss the effect of astrophysical uncertainties on the WIMP interpretation of the BERNABEI 1999 signal.


pdgid: S030DM2
text:
BELLI 1996C use background subtraction and obtain sigma<0.35 pb (<0.15 fb) (90% CL) for spin-dependent (independent) X0-proton cross section. The confidence level is from R. Bernabei, private communication, May 20, 1999.


pdgid: S030DM2
text:
REUSSER 1991 limit here is changed from published (0.3) after reanalysis by authors. J.L. Vuilleumier, private communication, March 29, 1996.


pdgid: S030DM3
text:
BERNABEI 1999D search for SIMPs (Strongly Interacting Massive Particles) in the mass range 10**3 -- 10**16 GeV. See their Fig. 3 for cross-section limits.


pdgid: S030DM3
text:
DERBIN 1999 search for SIMPs (Strongly Interacting Massive Particles) in the mass range 10**2 -- 10**14 GeV. See their Fig. 3 for cross-section limits.


pdgid: S030DM3
text:
BELLI 1996C use background subtraction and obtain sigma<0.7 pb (<0.7 fb) (90% CL) for spin-dependent (independent) X0-proton cross section. The confidence level is from R. Bernabei, private communication, May 20, 1999.


pdgid: S030DM3
text:
REUSSER 1991 limit here is changed from published (5) after reanalysis by authors. J.L. Vuilleumier, private communication, March 29, 1996.


pdgid: S030UDM
text:
ABE 2024A report Kamland-Zen search for de-excitation of WIMP DM bound to nucleus due to small mass splitting with charged WIMP partner. No signal observed. Limits placed in several parameter planes such as charged WIMP decay width vs. mass splitting (e.g. Fig. 7).


pdgid: S030UDM
text:
ARNQUIST 2024A report DAMIC-M search for MeV-scale DM scatter on e via mediator. No signal observed. Limits placed in sigma(e) vs m plane.


pdgid: S030UDM
text:
ABE 2023A search for boosted sub-GeV DM using 0.37 Mt.y exposure of SuperK data. No signal observed. Model dependent limits set, see Fig. 3 corrected in ABE 2023G erratum.


pdgid: S030UDM
text:
ADAMS 2023 search for inelastic DM scatter in fluorocarbons. No signal observed. Limits placed in sigma vs. m(chi) mass splitting plane.


pdgid: S030UDM
text:
ADHIKARI 2023B search for boosted heavy photon DM in MeV range using Cosine-100. No signal observed. Limits placed in coupling vs. mass plane for masses 1 -- 100 MeV.


pdgid: S030UDM
text:
AL-KHARUSI 2023 search for absorption of MeV-scale DM with 234.1 kg.y exposure of  Xe136, triggering beta decay. No signal observed. Limit placed in cross section vs. mass plane for m(chi) = 1.7 -- 11.6 MeV (see Fig. 5).


pdgid: S030UDM
text:
APRILE 2023 search for multiple scatter events from Planck scale-DM particles. No signal observed. Limits set on sigma^SI and sigma^SD on n and p.


pdgid: S030UDM
text:
HUANG 2023 search for MeV-scale scalar DM interacting via GeV-scale dark mediator. Limits placed on cross section vs. mass plane.


pdgid: S030UDM
text:
NING 2023A search for boosted LDM arising from eta decays which are produced in CR  events with 0.63 t.y exposure. No signal observed. Limits placed in sigma(chi N)  vs. m(chi) plane for various mediator models and branching fraction assumptions (see Fig. 2).


pdgid: S030UDM
text:
ADHIKARI 2022 search for multiple scatter of Planck scale DM on Ar using DEAP detector. No signal observed. Limits placed in mass vs. cross section plane for m(DM): E7 -- E19 GeV.


pdgid: S030UDM
text:
ADHIKARI 2022D report search for annual modulation signal of DM in a 173 kg.yr exposure of NaI; result consistent with both the modulation amplitude reported by DAMA/LIBRA and no-modulation.


pdgid: S030UDM
text:
DAI 2022A search for MeV-scale exotic DM interaction with Ge; no signal observed; limits set in m(DM) vs. cross section plane for m(DM) ~ 5 -- 60 MeV in simplified model.


pdgid: S030UDM
text:
GU 2022 use PANDAX to search for absorption of fermionic DM in MeV range in Xe; no  signal observed; limits set in m(DM) vs. cross section plane for m(DM) ~ 30 -- 125 MeV.


pdgid: S030UDM
text:
ZHANG 2022 search for light DM scatter on e; no signal observed; limits placed in  vs. m(DM) plane for m(DM) ~ 10 -- 180 keV.


pdgid: S030UDM
text:
AKERIB 2021B place limits on 15 WIMP non-relativistic EFT couplings for m(DM): 10 -- 4000 GeV  using 3.14 kg d exposure.


pdgid: S030UDM
text:
AMARE 2021 search for WIMP annual modulation signal on NaI target in the Canfranc Underground Laboratory (LSC). With an effective exposure of 313.95 kg y, and a sensitivity of 2.5 sigma no signal is observed. Incompatible with DAMA/LIBRA at 3.3 sigma level.


pdgid: S030UDM
text:
WANG 2021K use CDEX detector to search for WIMP dark matter scatter on Ge; no signal observed; limits placed on 14 non-relativistic effective operators along with WIMP-pion coupling for m(WIMP) ~ 3 -- 20 GeV.


pdgid: S030UDM
text:
AGOSTINI 2020 search for keV-MeV scale super-WIMP absorption in Ge in GERDA; no signal; limits placed on keV-MeV scale bosonic superWIMPs in coupling vs. mass plane.


pdgid: S030UDM
text:
ANDRIANAVALOMAHEFA 2020 search for hidden photon DM in eV range; place limits in m(DM) vs ln(chi) plane: exclude coupling chi ~< 1E-12 for m(DM) ~ 2.5 -- 7 eV.


pdgid: S030UDM
text:
CLARK 2020 use Majorana and Xe-1-ton data to constrain superheavy multply interacting dark matter (MIMP) in range m~ E8 -- E17 GeV depending on interaction cross section.


pdgid: S030UDM
text:
ABRAMOFF 2019 search for MeV scale DM via DM-e scattering and dark photon DM via absorption in Si; limits set in coupling vs. m(chi) plane and on dark photon in m(A) vs. kinetic mixing parameter plane.


pdgid: S030UDM
text:
ADHIKARI 2019 search for annual modulation signal from WIMP scatter on NaI with 1.7 yr exposure; result consistent with both DAMA/LIBRA and null hypothesis.


pdgid: S030UDM
text:
AMARE 2019 is ANAIS-112 search for WIMP scatter annual modulation on NaI; 157.55 kg yr exposure; result compatible with null hypothesis; confirm goal of reaching sensitivity at 3sigma to DAMA/LIBRA result in 5 years.


pdgid: S030UDM
text:
APRILE 2019 search for WIMP-pion scattering in Xe; no signal: require sigma(chi pi) < 6.4E-10 pb for m(chi) = 30 GeV.


pdgid: S030UDM
text:
BRINGMANN 2019 derive theoretically limits on GeV and sub-GeV mass dark matter, in its high energy component generated by interaction with cosmic rays; place limits on sigma^SI and sigma^SD < E5 pb.


pdgid: S030UDM
text:
BRUNE 2019 examine possibility of Majoron dark matter; limits placed on Majoron mass vs. coupling from SN1987a and nu-less double beta decay.


pdgid: S030UDM
text:
CHOI 2019 from multimessenger observation finds limit on sigma(nu chi)/m(DM) < 5.1E-23 cm**2/GeV based on 290 TeV IceCube neutrino event.


pdgid: S030UDM
text:
HA 2019 search for inelastic boosted MeV scale dark photon using COSINE-100 data; limits placed in m vs. epsilon plane for various mediators.


pdgid: S030UDM
text:
KLOPF 2019 search for DM via n --> chi e+ e-; no signal: limits placed in branching fraction vs. m(e+ e-) plane.


pdgid: S030UDM
text:
AARTSEN 2018D search for long-lived DM particles decaying chi --> nu X; no excess seen; for DM masses above 10 TeV, excluding lifetimes shorter than E28 s.


pdgid: S030UDM
text:
ABE 2018F search for keV mass ALPs and hidden photons (HP) scatter on electrons; limits set on mass vs. coupling.


pdgid: S030UDM
text:
AGNES 2018B search for MeV-scale DM scatter on electrons in Ar; no signal; require sigma(chi e) < 9E-3 pb for DM form factor F(DM) = 1 and < 300 pb for F(DM) proportional to 1/q**2 for m(chi) = 100 MeV.


pdgid: S030UDM
text:
AGNESE 2018B search for MeV scale DM via DM-e scattering and dark photon DM via absorption in Si; limits set on MeV DM in coupling vs. m(chi) plane and on dark photon in m(A^') vs. kinetic mixing plane.


pdgid: S030UDM
text:
AKERIB 2018A search for annual and diurnal modulation of DM scattering rate on electrons for recoil energy between 2 and 6 keVee; no signal found.


pdgid: S030UDM
text:
ARMENGAUD 2018 search for ALP from the Sun and galactic bosonic DM, interacting in Ge; no signal; limits set for 0.8 -- 500 keV DM particles.


pdgid: S030UDM
text:
KACHULIS 2018 search for an excess of elastically scattered electrons above the atmospheric neutrino background in Super-K; limits placed for simple annihilation or decay in the Sun or galactic center producing "boosted" dark matter.


pdgid: S030UDM
text:
AGUILAR-AREVALO 2017 search for hidden photon DM scatter on Si target CCD; limit kinetic mixing kappa < 1E-12 for m = 10 eV.


pdgid: S030UDM
text:
APRILE 2017D set limits on 14 WIMP-nucleon different interaction operators. No deviations found using 225 live days in the 6.6 -- 240 keV recoil energy range.


pdgid: S030UDM
text:
APRILE 2017H search for keV bosonic DM via e chi --> e, looking for electronic recoils with 224.6 live days of data and 34 kg of LXe. Limits set on chi e e coupling for m(chi) = 8 -- 125 keV.


pdgid: S030UDM
text:
APRILE 2017K search for magnetic inelastic DM via chi N --> chi^* --> chi gamma. Limits set in DM magnetic moment vs. mass splitting plane for two DM masses corresponding to the DAMA/LIBRA best fit values.


pdgid: S030UDM
text:
ANGLOHER 2016A require q**2 dependent scattering < 8E-3 pb for asymmetric DM m(WIMP) = 3 GeV on CaWO(4) target. It uses a local dark matter density of 0.38 GeV/cm**3.


pdgid: S030UDM
text:
APRILE 2015 search for periodic variation of electronic recoil event rate in the data between Feb. 2011 and Mar. 2012. No significant modulation is found for periods up to 500 days.


pdgid: S030UDM
text:
APRILE 2015A search for X0 scattering off electrons. See their Fig. 4 for limits on cross section through axial-vector coupling for mass(X0) between 0.6 GeV and 1 TeV. For mass(X0) = 2 GeV, sigma< 60 pb (90%CL) is obtained.


pdgid: S030DMA
text:
ACHARYYA 2024 search for TeV-scale wimp annihilation in dwarf spheroidals. No signal observed. Limits placed on <> vs. m(wimp) in various annihilation channels. Quoted limit for chi chi --> W W.


pdgid: S030DMA
text:
CAO 2024 search for superheavy WIMP annihilation in dwarf spheroidals to b bbar or tau taubar. No signal observed. Limits set in <> vs. m(WIMP) plane. Quoted limit for b bbar with m(WIMP) = 1 TeV.


pdgid: S030DMA
text:
CHOLIS 2024 derive limits on wimp annihilation contribution to Fermi-LAT observation of isotropic gamma ray background. Limits set in <> vs m plane for various chi chi annihilation channel.


pdgid: S030DMA
text:
CRNOGORCEVIC 2024 interpret published Fermi-LAT data aimed at Ursa-Major III to derive limits on WIMP annihilation in high J-factor dwarf spheroidal. Fermi-LAT limits are recast in <> vs m plane depend on J and on assumed annihilation channel.


pdgid: S030DMA
text:
DE-LA-TORRE-LUQUE 2024 analyze 15 years Fermi-LAT data for m(WIMP) 10 -- 300 GeV annihilation to photons. No signal observed. Limits placed in <> vs m plane for several models motivated by galactic center excess.


pdgid: S030DMA
text:
MANNA 2024 analyze SPT-SZ survay for 1 -- 300 GeV gamma rays from wimp annihilation in galaxy clusters. Some slight signals observed in conflict with dwarf spheroidal searches. Limits in <> vs m plane; quoted limit is for m(wimp) = 10 GeV in b bbar annihilation channel.


pdgid: S030DMA
text:
MCDANIEL 2024 combined 14.3 years Fermi-LAT data from multiple dwarf spheroidals to gain updated bounds on WIMP annihilation rates with some 2sigma excesses claimed. Reported limit is for 100 GeV WIMP mass.


pdgid: S030DMA
text:
MCDANIEL 2024 perform combined 14 year Fermi-LAT analysis of gammas from dwarf spheroidals. New limits obtained from Fig. 6. Quoted value for m(WIMP) = 100 GeV in b bbar and tau taubar annihilation channels.


pdgid: S030DMA
text:
SONG 2024 use Fermi-LAT data to constrain heavy E3 -- E11 GeV DM annihilation and decay. Limits placed in <> vs. m and lifetime vs. m planes.


pdgid: S030DMA
text:
SONG 2024A examine Fermi-LAT gamma ray data from superheavy WIMP annihilation/decay in galaxy clusters. Limits placed in <> vs m and lifetime vs m planes for a variety of annihilation/decay modes.


pdgid: S030DMA
text:
ZAKHAROV 2024A derive limits DM annihilation to X-rays in the 4 -- 15 keV particle mass range via SRG/ART-XC telescope. Limits placed in <> vs m plane. Quoted limit is from MW halo for m = 10 keV, see Fig. 10.


pdgid: S030DMA
text:
ABBASI 2023A search for WIMP-WIMP annihilation to nu's. No signal observed. Require <> < E-24 cm**3/s for m(chi) ~ 10 -- 10E4 GeV for various halo profiles.


pdgid: S030DMA
text:
ABBASI 2023B search for PeV-scale WIMP-WIMP annihilation to mu or b pairs. No signal observed. Require <> < E-22 cm**3/s for chi chi --> b bbar with m(chi) about 1 PeV or <> < E-23 cm**3/s for chi chi --> mu+ mu- with m(chi) about 1 PeV.


pdgid: S030DMA
text:
ABE 2023B search for WMP-WIMP annihilation to gamma in GC. No signal observed. Require <> < 5E-28 cm**3/s for m(chi) = 1 TeV or <> < 1E-25 cm**3/s for m(chi) = 100 TeV.


pdgid: S030DMA
text:
ALBERT 2023 search for WIMP pair annihilation to gamma in galactic halo. No signal observed. Limits placed in <> vs. mass (10 -- 100 TeV) plane for various annihilation channels.


pdgid: S030DMA
text:
CHENG 2023A provide updated combined Fermi-LAT/DAMPE search for gamma line from WIMP annihilation. No signal observed. Limits placed in <> vs. mass (6 -- 200 GeV) plane for various halo profiles.


pdgid: S030DMA
text:
FOSTER 2023 search for gamma ray line in Fermi-LAT data. No signal observed. Limits placed in <> vs. m(chi) plane. For Higgsino DM limit see Fig. 12.


pdgid: S030DMA
text:
GUO 2023 search with Five-hundred-meter Aperture Spherical Radio Telescope for synchrotron emission radio signal of DM annihilation from dwarf spheroidal galaxy. No signal observed. Limits set in <> vs. m(chi) plane for various annihilation final states.


pdgid: S030DMA
text:
GUO 2023A search in public IceCube data for DM annihilation to neutrinos. No signal observed. Limits placed in <> vs m(chi) plane for various annihilation assumptions.


pdgid: S030DMA
text:
LAVIS 2023 search for 2HDM+S DM and generic spectra using MeerKAT. No signal observed. Limits placed in <> vs. mass (10 -- 1000 GeV) plane for various annihilation channels.


pdgid: S030DMA
text:
ABDALLA 2022 search for WIMP annihilation in galactic center to gamma rays using HESS; no  signal observed; limits set in mass vs <> plane for dominant annihilation to W W or  tau taubar. Limit here for tau taubar channel 0.7 TeV mass.


pdgid: S030DMA
text:
ALBERT 2022A search for secluded PeV-scale DM annihilation to four final states; no signal detected; limits placed in <> vs. m(chi) plane for m(chi): 6 -- 6000 TeV for m(mediator) = 50, 250, and 1000 GeV.


pdgid: S030DMA
text:
CHAN 2022 derive a variety of limits on DM annihilation to various channels resulting in X-rays from dwarf galaxy Omega Centauri. Limits are very dependent on assumed DM density and diffusion coefficient. Quoted limit is for m(WIMP) = 100 GeV annihilating to W W with parameters as in Fig. 4.


pdgid: S030DMA
text:
EGOROV 2022 derives limits on DM annihlation to b bbar or tau taubar via radio  signals from M31; quoted limit from b bbar channel with LOFAR telescope as main data source, using parameters as in Fig. 10 (green  curve) for m(chi) = 100 GeV.


pdgid: S030DMA
text:
MANCONI 2022 use polarized synchrotron emission data from Planck to constrain WIMP  annihilation cross section in Galaxy; limits set in <> vs. m(DM) plane.


pdgid: S030DMA
text:
ABDALLAH 2021 search for WIMP-WIMP annihilation into 2 monoenergetic gamma rays in WLM dwarf irregular galaxy using HESS data. No signal. Limits placed in <> vs. m(WIMP) plane for a mass of 370 GeV.


pdgid: S030DMA
text:
CIRELLI 2021 derive limits on light DM annihilation to e e, mu mu, pi pi that then produce X-rays using data published by INTEGRAL telescope. Limits placed in <> vs. m(DM) plane for m(DM) = 1 -- 5000 MeV.


pdgid: S030DMA
text:
JOHN 2021 derive limits on leptophilic DM annihilating to positrons by comparing expected spectra to AMS-02 data. The range m(DM): 60 -- 300 GeV appears excluded for this type of model, see Fig. 3.


pdgid: S030DMA
text:
ABAZAJIAN 2020 derive new limits on WIMP annihilation in galactic center (GC):  <> < 2.5E-27 cm**3/s for m(WIMP) = 50 GeV: seems to rule out WIMP explanation for GC gamma excess, favouring an astrophysics origin.


pdgid: S030DMA
text:
ABDALLAH 2020 search for WIMP annihilation in newly discovered by DES dwarf satellite galaxies using HESS; limits placed in <> vs. m(DM) plane depending on annihilation channel and which dwarf satellite.


pdgid: S030DMA
text:
ABE 2020G search Super-Kamiokande data for WIMP annihilation to neutrinos in galactic center/halo; no signal; limits placed in <> vs. m(DM) plane depending on annihilation channel and m(WIMP). Reported limit for annihilation to nu nubar at 1 GeV.


pdgid: S030DMA
text:
ALBERT 2020 search for TeV-scale WIMP annihlation to gamma gamma in dwarf spheroidal galaxies; no signal; limits placed in vs m(WIMP) plane: e.g. < 2.2E-24 cm**3/s for m(WIMP) = 1 TeV.


pdgid: S030DMA
text:
ALBERT 2020A search for WIMP annihilation to nus in galactic center using Antares; limits placed in sigma.v vs m(WIMP) plane e.g. sigma.v < 5E-24 cm**3/s for m(WIMP) = 1 TeV assuming annihilation dominantly to tau taubar.


pdgid: S030DMA
text:
ALBERT 2020C report combined Antares + IceCube search for WIMP annihilation to tau taubar; for NFW halo profile report < 1E-23 cm**3/s for m(WIMP) = 100 GeV.


pdgid: S030DMA
text:
ALVAREZ 2020 use profiling over J-factor distributions and background to derive new limits on sigma.v; e.g. sigma.v < 8E-26 cm**3/s for m(WIMP) = 100 GeV.


pdgid: S030DMA
text:
HOOF 2020 examine gamma rays from 27 dwarf spheroidals using Fermi-LAT data; place limits in sigma.v vs m(WIMP) plane using profile likelihood and marginalized posterior techniques for DM annihilation to tau taubar and b bbar; quoted limit uses first technique and b bbar channel for m(WIMP) = 100 GeV; results rule out WIMP explanation of galactic center excess.


pdgid: S030DMA
text:
MAZZIOTTA 2020 use Fermi-LAT pointed-at-Sun data to search for DM annihilation in the Sun to long-lived mediators decaying into gamma rays, i.e. chi chi --> phi phi --> 4 gamma. Limits placed on the SI and SD DM-nucleon cross sections in the sigma-DM mass plane for DM masses in the range 3 GeV - 1.8 TeV. Limits are evaluated in both cases of equilibrium and non-equilibrium.


pdgid: S030DMA
text:
ABEYSEKARA 2019 search for gammas from DM annihilation in galactic substructures with HAWC; no signal, limits placed in J<> vs. declination plane for m(DM) ~ 1 -- 108 TeV.


pdgid: S030DMA
text:
ALBERT 2019B search for DM signal from M31 galaxy in mu, tau, t, b, W channels using HAWC for m(DM) ~ 1 -- 100 TeV; no signal, limits placed in <> vs. m(DM) plane.


pdgid: S030DMA
text:
CHEUNG 2019 derive model-dependent bounds on <> from EDGES data: < 4E-26 cm**3/s for e+ e- and b bbar for m(chi) = 100 GeV (including boost factor).


pdgid: S030DMA
text:
DI-MAURO 2019 place limits on WIMP annihilation via Fermi-LAT observation of M31 and M33 galaxies: <> < 7E-27cm**3/s for m(chi) = 20 GeV from M31.


pdgid: S030DMA
text:
JOHNSON 2019 search for gamma-rays, 10 -- 600 GeV energy, from P-wave annihilating DM around SgrA* BH using Fermi-LAT; limits set for various models.


pdgid: S030DMA
text:
LI 2019D search for chi chi --> gamma in Fermi-LAT data; no signal, require <> < 2E-26 cm**3/s for m(chi) = 100 GeV.


pdgid: S030DMA
text:
NG 2019 search for X-ray line from sterile nu decay/annihilation using NuStar M-31; no signal: limits placed in m(nu) vs mixing angle and <> vs m(nu).


pdgid: S030DMA
text:
QUEIROZ 2019 examine chi chi --> chi SM semi-annihilation of DM reaction; limits placed for various assumed SM particles in <> vs. m(chi) plane.


pdgid: S030DMA
text:
ABDALLAH 2018 search for WIMP WIMP gamma X in central galactic halo, 10 years of data; limits placed in <> vs. m(WIMP) plane for m(WIMP): 0.3 -- 70 TeV.


pdgid: S030DMA
text:
AHNEN 2018 search for WIMP WIMP --> gamma X from Ursa Major II; limits set in <> vs. m(WIMP) plane for b bbar, W+ W-, tau+ tau-, and mu+ mu- annihilation modes.


pdgid: S030DMA
text:
ALBERT 2018B search for TeV-scale WIMPs with WIMP WIMP --> gamma X in Andromeda galaxy using HAWC Observatory; limits set in <> vs m(WIMP) plane.


pdgid: S030DMA
text:
CHANG 2018A examine chi chi --> b bbar --> gamma using Fermi Pass 8 data; no signal; require <> < E-26 cm**3/s for m(chi) = 50 GeV.


pdgid: S030DMA
text:
LISANTI 2018 examine Fermi Pass 8 gamma-ray data from galaxy groups; report m(WMP) > 30 GeV for annihilation in b bbar channel.


pdgid: S030DMA
text:
MAZZIOTTA 2018 examine Fermi-LAT electron and positron spectra searching for features originating from DM particles annihilation into e+ e- pairs, from 45 GeV to 2 TeV; no signal found, limits are obtained.


pdgid: S030DMA
text:
AARTSEN 2017C use 1005 days of IceCube data to search for chi chi --> neutrinos via various annihilation channels. Limits set.


pdgid: S030DMA
text:
ALBERT 2017A search for DM annihilation to nus using ANTARES data from 2007 -- 2015. No signal. Limits set in <> vs. m(DM) plane for m(DM) ~10 -- 10E5 GeV. The listed limit is for m(DM) = 100 TeV.


pdgid: S030DMA
text:
ARCHAMBAULT 2017 set limits for WIMP mass between 100 GeV and 1 TeV on <> for W+ W-, Z Z, b bbar, s sbar, u ubar, d dbar, t tbar, e+ e-, g g, c cbar, h h, gamma gamma, mu+ mu-,tau+ tau- annihilation channels.


pdgid: S030DMA
text:
AVRORIN 2017 find upper limits for the annhilation cross section in various channels for DM particle mass between 30 GeV and 10 TeV. Strongest upper limits coming from the two neutrino channel require <> < 6E-20 cm**3/s in dwarf galaxies and <> < 7E-21 cm**3/s in LMC for 5 TeV WIMP mass.


pdgid: S030DMA
text:
BOUDAUD 2017 use data from the spacecraft Voyager 1, beyond the heliopause, and from AMS02 on chi chi --> e+ e- to require <><1.E-28 cm**3/s for m(chi) = 10 MeV.


pdgid: S030DMA
text:
ABDALLAH 2016 require <> < 6E-26 cm**3/s for m(WIMP) = 1.5 TeV from 254 hours observation (W W channel) and < 2E-26 cm**3/s for m(WIMP) = 1.0 TeV in tau+ tau- channel.


pdgid: S030DMA
text:
ABDALLAH 2016A search for line spectra from WIMP + WIMP gamma gamma in 18 hr HESS data; rule out previous 130 GeV WIMP hint from Fermi-LAT data.


pdgid: S030DMA
text:
AVRORIN 2016 require <s.v> < 1.91E-21 cm**3/s from WIMP annihilation to nus via W W channel for m(WIMP) = 1 TeV.


pdgid: S030DMA
text:
CAPUTO 2016 place limits on WIMPs from annihilation to gamma rays in Small Magellanic Cloud using Fermi-LaT data: <><3E-26cm**3/s for m(WIMP) = 10 GeV.


pdgid: S030DMA
text:
FORNASA 2016 use anisotropies in the gamma-ray diffuse emission detected by Fermi-LAT to bound <> < 10**-25cm**3/s for m(WIMP) = 100 GeV in b bbar channel: see Fig. 28. The limit is driven by dark-matter subhalos in the Milky Way and it refers to their Most Constraining Scenario.


pdgid: S030DMA
text:
LEITE 2016 constrain WIMP annihilation via search for radio emissions from Smith cloud; <> < 5E-27cm**3/s in e e channel for m(WIMP) = 5 GeV.


pdgid: S030DMA
text:
LI 2016 re-analyze Fermi-LAT data on 8 dwarf spheroidals; set limit <><2E-26 cm**3/s for m(WIMP) = 100 GeV in b bbar mode with substructures included.


pdgid: S030DMA
text:
LI 2016A constrain <> < 10**-25cm**3/s in b bbar channel for m(WIMP) = 100 GeV using Fermi-LAT data from M31; see Fig. 6.


pdgid: S030DMA
text:
LIANG 2016 search dwarf spheroidal galaxies, Large Magellanic Cloud, and Small Magellanic Cloud for gamma-line in Fermi-LAT data.


pdgid: S030DMA
text:
LU 2016 re-analyze Fermi-LAT and AMS-02 data; require <> <E-25cm**3/s for mass(m)(WIMP) = 1 TeV in b bbar channel.


pdgid: S030DMA
text:
SHIRASAKI 2016 re-anayze Fermi-LAT extra-galactic data; require <><E-23cm**3/s for m(WIMP) = 1 TeV in b bbar channel; see Fig. 8.


pdgid: S030DMA
text:
AARTSEN 2015C search for neutrinos from X0 annihilation in the Galactic halo. See their Figs. 16 and 17, and Table 5 for limits on sigma.v for X0 mass between 100 GeV and 100 TeV.


pdgid: S030DMA
text:
AARTSEN 2015E search for neutrinos from X0 annihilation in the Galactic center. See their Figs. 7 and 9, and Table 3 for limits on sigma.v for X0 mass between 30 GeV and 10 TeV.


pdgid: S030DMA
text:
ABRAMOWSKI 2015 search for gamma from X0 annihilation in the Galactic center. See their Fig. 4 for limits on sigma.v for X0 mass between 250 GeV and 10 TeV.


pdgid: S030DMA
text:
ACKERMANN 2015 search for monochromatic gamma from X0 annihlation in the Galactic halo. See their Fig. 8 and Tables 2 -- 4 for limits on sigma.v for X0 mass between 0.2 GeV and 500 GeV.


pdgid: S030DMA
text:
ACKERMANN 2015A search for gamma from X0 annihilation (both Galactic and extragalactic) in the isotropic gamma background. See their Fig. 7 for limits on sigma.v for X0 mass between 10 GeV and 30 TeV.


pdgid: S030DMA
text:
ACKERMANN 2015B search for gamma from X0 annihilation in 15 dwarf spheroidal satellite galaxies of the Milky Way. See their Figs. 1 and 2 for limits on sigma.v for X0 mass between 2 GeV and 10 TeV.


pdgid: S030DMA
text:
ADRIAN-MARTINEZ 2015 search for neutrinos from X0 annihilation in the Galactic center.  See their Figs. 10 and 11 and Tables 1 and 2 for limits on sigma.v for X0 mass between 25 GeV and 10 TeV.


pdgid: S030DMA
text:
ACKERMANN 2014 search for gamma from X0 annihilation in 25 dwarf spheroidal satellite galaxies of the Milky Way. See their Tables II--VII for limits assuming annihilation into e+ e-, mu+ mu-, tau+ tau-, u ubar, b bbar, and W+ W-, for X0 mass ranging from 2 GeV to 10 TeV.


pdgid: S030DMA
text:
ALEKSIC 2014 search for gamma from X0 annihilation in the dwarf spheroidal galaxy Segue 1. The listed limit assumes annihilation into W+ W-. See their Figs. 6, 7, and 16 for limits on sigma.v for annihilation channels mu+ mu-, tau+ tau-, b bbar, t tbar, gamma gamma, gamma Z, W+ W-, Z Z for X0 mass between 10**2 and 10**4 GeV.


pdgid: S030DMA
text:
AARTSEN 2013C search for neutrinos from X0 annihilation in nearby galaxies and galaxy clusters. See their Figs. 5 -- 7 for limits on sigma.v for X0 X0 --> nu nubar, mu+ mu-, tau+ tau-, and W+ W- for X0 mass between 300 GeV and 100 TeV.


pdgid: S030DMA
text:
ABRAMOWSKI 2013 search for monochromatic gamma from X0 annihilation in the Milky Way halo in the central region. Limit on sigma.v between 10**-28 and 10**-25 cm**3 s**-1 (95% CL) is obtained for X0 mass between 500 GeV and 20 TeV for X0 X0 --> gamma gamma. X0 density distribution in the Galaxy by Einasto is assumed. See their Fig. 4.


pdgid: S030DMA
text:
ACKERMANN 2013A search for monochromatic gamma from X0 annihilation in the Milky Way. Limit on sigma.v for the process X0 X0 --> gamma gamma in the range 10**-29 -- 10**-27 cm**3 s**-1 (95% CL) is obtained for X0 mass between 5  and 300 GeV. The limit depends slightly on the assumed density profile of X0 in the Galaxy. See their Tables VII-X and Fig.10. Supersedes ACKERMANN 2012.


pdgid: S030DMA
text:
ABRAMOWSKI 2012 search for gamma's from X0 annihilation in the Fornax galaxy cluster. See their Fig. 7 for limits on sigma.v for X0 mass between 0.1 and 100 TeV for the annihilation channels tau+ tau-, b bbar, and W+ W-.


pdgid: S030DMA
text:
ACKERMANN 2012 search for monochromatic gamma from X0 annihilation in the Milky Way. Limit on sigma.v in the range E-28 -- E-26 cm**3s**-1 (95% CL) is obtained for X0 mass between 7 and 200 GeV if X0 annihilates into gamma gamma. The limit depends slightly on the assumed density profile of X0 in the Galaxy. See their Table III and Fig. 15.


pdgid: S030DMA
text:
ACKERMANN 2012 search for gamma from X0 annihilation in the Milky Way in the diffuse gamma background. Limit on sigma.v of E-24 cm**3s**-1 or larger is obtained for X0 mass between 5 GeV and 10 TeV for various annihilation channels including W+ W-, b bbar, g g, e+ e-, mu+ mu-, tau+ tau-. The limit depends slightly on the assumed density profile of X0 in the Galaxy. See their Figs. 17 -- 20.


pdgid: S030DMA
text:
ALIU 2012 search for gamma's from X0 annihilation in the dwarf spheroidal galaxy Segue 1. Limit on sigma.v in the range 10**-24 -- 10**-20 cm**3s**-1 (95% CL) is obtained for X0 mass between 10 GeV and 2 TeV for annihilation channels e+ e-, mu+ mu-, tau+ tau-, b bbar, and W+ W-. See their Fig. 3.


pdgid: S030DMA
text:
ABBASI 2011C search for nu_{{mu}} from X0 annihilation in the outer halo of the Milky Way. The limit assumes annihilation into nu nu. See their Fig. 9 for limits with other annihilation channels.


pdgid: S030DMA
text:
ABRAMOWSKI 2011 search for gamma from X0 annihilation near the Galactic center. The limit assumes Einasto DM density profile.


pdgid: S030DMA
text:
ACKERMANN 2011 search for gamma from X0 annihilation in ten dwarf spheroidal satellite galaxies of the Milky Way. The limit for m = 10 GeV assumes annihilation into b bbar, the others W+ W-. See their Fig. 2 for limits with other final states. See also GERINGER-SAMETH 2011 for a different analysis of the same data.


pdgid: S030DMP
text:
AAD 2024AC search for t tbar + mediator, where mediator decays to dark matter, within 140 fb**-1 of data. No signal observed. Limits placed in sigma vs m(mediator) plane.


pdgid: S030DMP
text:
AAD 2024AC search for t tbar+MET signal at sqrt(s)=13 TeV and 139 fb**-1. No signal observed. Assume DM mediator model coupling to t tbar and limits placed in various m(DM), m(mediator), coupling planes.


pdgid: S030DMP
text:
AAD 2024AH search for SUSY in pMSSM model. No signal observed. Several regions of DM-allowed parameters space now ruled out.


pdgid: S030DMP
text:
AAD 2024AK search for top + MET in various simplified models including mediator decaying to DM. No signal observed. Limits placed in various parameter space planes.


pdgid: S030DMP
text:
AAD 2024CD search for hadronically-decaying W / Z plus MET events in 140 fb**-1 at 13 TeV. No signal observed. Limits placed in m(chi) vs. mediator mass plane for simplified dark matter model.


pdgid: S030DMP
text:
HAYRAPETYAN 2024B search for inelastic DM production where heavier state decays to displaced muons. No signal observed. Limits placed in signal strength vs mass plane for various choices of mass gap.


pdgid: S030DMP
text:
HAYRAPETYAN 2024W search for dark matter via dark Higgs decay in W W + MET events. No signal observed. Limits placed in m(chi) vs m(mediator) or m(s) plane where s is dark Higgs.


pdgid: S030DMP
text:
AAD 2023A search for H --> invisible. No signal observed. Results interpreted in terms of several DM Higgs portal simplified models.


pdgid: S030DMP
text:
AAD 2023AF search for tbar t + H --> invisible with 139 fb**-1 of data. No signal observed. Limits placed on branching fractions of H decays etc. for various DM mediator models. Result also included in AAD 2023A.


pdgid: S030DMP
text:
AAD 2023AJ search for t W chi chi production in mediator-extended 2HDM with 139 fb**-1 of data. No signal observed. Limits placed in m(H) vs. m(mediator) and tan(beta) vs. m(H) planes.


pdgid: S030DMP
text:
AAD 2023BX search for A --> H a production where H --> tau taubar and a --> chi chi. No signal observed. Limits placed on 2HDM+a model.


pdgid: S030DMP
text:
AAD 2023W search for DM in dark Higgs model via W W chi chi final state with 139 fb**-1 of data. No signal detected. Limits set in m(dark Higgs) vs. m(Z^') plane.


pdgid: S030DMP
text:
AKIMOV 2023 search for light DM via COHERENT CsI detector at SNS. No signal observed. For scalar DM model, limits set for m(chi) = 1 -- 300 MeV. Limit of CS(chi N) < 1E1 pb set at peak sensitivity m(chi) = 25 MeV.


pdgid: S030DMP
text:
LIN 2023C search for chi --> gamma gamma decay where p --> chi chi at KOTO. No  signal observed. Limits placed on K(L)0 branching fraction.


pdgid: S030DMP
text:
AAD 2022D search for Z+H production with Z --> l lbar and H --> chi chi with  139 fb**-1 at 13 TeV; no signal found; limits placed in various simplified models depending on Higgs  portal and DM mediator.


pdgid: S030DMP
text:
AAD 2022P search for H production via VBF with H --> chi chi with 139 fb**-1 at 13 TeV; no signal found; limits placed for various Higgs DM portal simplified models.


pdgid: S030DMP
text:
AGUILAR-AREVALO 2022A report search for MeV vector portal and leptophobic DM via scatter on liquid Ar at the Lujan stopped pion source at LANL; no signal detected; limits placed on vector portal and leptophobic DM vs. m(chi): 1 -- 40 MeV.


pdgid: S030DMP
text:
TUMASYAN 2022AA search for Z^' decay to dark quarks with 138 fb**-1 at 13 TeV; no  signal observed; limits exclude a wide range of strongly coupled hidden sector models.


pdgid: S030DMP
text:
TUMASYAN 2022AG search for strongly interacting dark matter production via scalar mediator, with SIMP decay to trackless jets with 16.1 fb**-1 at 13 TeV; no signal detected; limits placed in mass vs. cross section plane for simplified models.


pdgid: S030DMP
text:
TUMASYAN 2022G search for VBF production of Higgs with H --> chi chi with 101 fb**-1 at 13 TeV, combined with earlier searches, in total 19.7 fb**-1 at 8 TeV and 140 fb**-1 at 13 TeV are used; no signal detected; limits placed in mass vs. cross section plane for various Higgs portal simplified models.


pdgid: S030DMP
text:
AAD 2021AZ search for DM in H notET gamma gamma notET events with 139  fb**-1 at 13 TeV. No signal observed. Limits placed for several simplified models.


pdgid: S030DMP
text:
AAD 2021BB search for DM in H notET b bbar notET events with 139 fb**-1 at 13 TeV. No signal observed. Limits placed for several simplified models.


pdgid: S030DMP
text:
AAD 2021D search for V V + chi chi, V --> q qbar with 139 fb**-1 at 13 TeV LHC. No signal detected. Limits placed in dark Higgs boson mass vs. m(Z^') plane. Here V V stand for W+- W-+, Z Z.


pdgid: S030DMP
text:
AAD 2021F search for monojet recoiling against invisibles with 139 fb**-1 at 13 TeV LHC. No signal detected. Limits placed in various simplified dark matter models.


pdgid: S030DMP
text:
AAD 2021K search for a photon recoiling against dark matter with 139 fb**-1 at 13 TeV LHC. No signal detected. Limits placed on parameter space of various simplified models.


pdgid: S030DMP
text:
AAD 2021O search for lepton + jets + notET to search for t-pairs + DM particles with 139 fb**-1 at LHC 13 TeV LHC. No signal detected. Limits placed in the cross-section vs.  mediator mass plane, assuming light DM states.


pdgid: S030DMP
text:
AAD 2021P search for lepton+ lepton- + jets + notET in context of various BSM models with 139 fb**-1 at 13 TeV LHC. No signal observed. Limits placed in parameter space of dark matter models and SUSY.


pdgid: S030DMP
text:
AAD 2021S search for b-jets + notET signal from BSM/DM models with 139 fb**-1 at 13 TeV LHC. No signal observed. Limits placed on parameter space of DM models.


pdgid: S030DMP
text:
SIRUNYAN 2021A search for DM production in association with leptonically decaying Z boson in 137 fb**-1 at 13 TeV; no signal; limits set in large variety of simplified DM models.


pdgid: S030DMP
text:
TUMASYAN 2021D search for DM and other exotica at CMS in jets + notET events with 137  fb**-1 at 13 TeV. No signal observed. Limits placed for a variety of simplified models.


pdgid: S030DMP
text:
SIRUNYAN 2020X search for DM in p p --> Z^' --> A ( Z^' ) h --> h + notET in CMS at 13 TeV with 35.9 fb**-1; no signal; limits placed in sigma^SI vs. m(chi), and sigma, m(A) and tanbeta vs m(Z') for considered DM models.


pdgid: S030DMP
text:
AABOUD 2019AA searches for BSM physics in more than 700 event classes with more than 10**5 regions at 13 TeV with 3.2 fb**-1; no significant signal.


pdgid: S030DMP
text:
AABOUD 2019AI searches for vector boson fusion p p --> H q q, H --> invisible at 13 TeV with 36.1 fb**-1; no signal: require B(H --> invisible) < 0.37 (0.28 expected).


pdgid: S030DMP
text:
AABOUD 2019AL perform search in three different channels for H --> chi chi at 7, 8 and 13 TeV; combined result BF(H --> invisible) < 0.26 (0.17 expected).


pdgid: S030DMP
text:
AABOUD 2019Q search for single t + notET at 13 TeV with 36.1 fb**-1 of data; no signal; limits set in sigma or coupling vs. mass plane for simplified models.


pdgid: S030DMP
text:
AABOUD 2019V review ATLAS results from 7, 8 and 13 TeV searches for mediator-based DM and DE scalar which couples to gravity; no signal: limits set for large variety of simplified models.


pdgid: S030DMP
text:
BANERJEE 2019 search for dark photon via e N --> e N+notE in NA64; no signal, limits placed in kinetic mixing epsilon vs. m(DM) plane for m(DM) ~ 0.001 -- 1 GeV.


pdgid: S030DMP
text:
SIRUNYAN 2019AN search at 13 TeV with 35.9 fb**-1 for p p --> H chi chi --> b bbar notET; no signal: limits set in the context of a 2HDM + pseudoscalar (a) model and a baryonic Z^' model.


pdgid: S030DMP
text:
SIRUNYAN 2019BC search for DM via LeptoQuark pair annihilation LQ LQ mu j chi chi --> mu j notET with 77.4 fb**-1, 13 TeV; no signal: limits placed in m(chi) vs. m(LQ) plane. Model dependent limits on DM mass up to 600 GeV depending on m(LQ) placed.


pdgid: S030DMP
text:
SIRUNYAN 2019BO search for vector boson fusion V V --> q q H with H --> chi chi at 13 TeV with 38.2 fb**-1; no signal: limits placed for several models. Also search for H --> invisible at 7, 8, and 13 TeV; no signal: limit placed on BF < 0.19.


pdgid: S030DMP
text:
SIRUNYAN 2019C search for DM via p p --> t tbar chi chi at 13 TeV, 35.9 fb**-1; no signal; limits placed on coupling vs. mediator mass for various simplified models.


pdgid: S030DMP
text:
SIRUNYAN 2019O search for p p --> gamma at 13 TeV with 35.9 fb**-1; no signal: limits placed on parameters of various models.


pdgid: S030DMP
text:
SIRUNYAN 2019X search for p p --> t tbar notET and p p --> t notET +... at 13 TeV with 35.9 fb**-1; no signal: limits placed on chi production sigma for various simplified models with m(chi) = 1 GeV.


pdgid: S030DMP
text:
AABOUD 2018 search for p p --> Z + notET with Z --> lepton lepton at 13 TeV with 36.1 fb**-1 of data. Limits set for simplified models.


pdgid: S030DMP
text:
AABOUD 2018A search for p p --> t tbar notET or p p --> b bbar notET at 13 TeV, 36.1 fb**-1 of data. Limits set for simplified models.


pdgid: S030DMP
text:
AABOUD 2018CA search for p p --> V chi chi with V --> j j at 13 TeV, 36.1 fb**-1. No signal observed. Limits set in m(DM) vs m(mediator) simplified model plane.


pdgid: S030DMP
text:
AABOUD 2018I search for p p --> j + notET at 13 TeV with 36.1 fb**-1 of data. Limits set for simplified models with pair-produced weakly interacting dark-matter candidates.


pdgid: S030DMP
text:
AGUILAR-AREVALO 2018B search for WIMP production in MiniBooNE p beam dump; no signal; limits set for m(chi) ~ 5 -- 50 MeV in vector portal DM model.


pdgid: S030DMP
text:
KHACHATRYAN 2018 search for p p --> Z(lepton lepton) + notET. No signal observed. Llimits set on effective dark matter interactions and other exotic physics models.


pdgid: S030DMP
text:
SIRUNYAN 2018BF search for p p --> t notET at 13 TeV and 36 fb**-1; no signal; limits placed on DM models involving a flavor changing neutral current, scalar resonance decaying to top quark and DM.


pdgid: S030DMP
text:
SIRUNYAN 2018BO search for high mass dijet resonances at 13 TeV and 36 fb**-1; no signal: limits placed on various models, including simplified DM models involving a spin = 1 Z^' mediator.


pdgid: S030DMP
text:
SIRUNYAN 2018BV search for p p --> Z notET at 13 TeV; no signal, limits placed for various exotic physics models including DM.


pdgid: S030DMP
text:
SIRUNYAN 2018C search for new physics in p p --> final states with two oppositely charged leptons at 13 TeV with 35.9 fb**-1. Limits placed on m(mediator) and top squark for various simplified models.


pdgid: S030DMP
text:
SIRUNYAN 2018CU search for p p --> Z notET at 13 TeV and 2.3 fb**-1. No signal observed. Limits placed for various exotic models including DM.


pdgid: S030DMP
text:
SIRUNYAN 2018DH search for p p --> chi chi h; h --> gamma gamma or tau taubar at 13 TeV, 35.9 fb**-1; no signal; limits placed on massive boson mediator Z^' in the context of Z^'+2HDM and baryonic Z^' models. Limits also cast in terms of spin-independent WIMP-nucleon cross section for masses 1 -- 200 GeV.


pdgid: S030DMP
text:
SIRUNYAN 2018S search for p p --> jets notET at 13 TeV; no signal: limits placed on simplified dark matter models, on the branching ratio of the Higgs boson to invisible particles, and on several other exotic physics models including fermion portal DM.


pdgid: S030DMP
text:
AABOUD 2017A search for H --> b bbar + notET. See Fig. 4b for limits set on VB mediator vs WIMP mass.


pdgid: S030DMP
text:
AABOUD 2017AM search for p p --> Z^' --> A h --> h (b bbar) + notET at 13 TeV. Limits set in m(Z^') vs. m(A) plane and on the visible cross section of h (b bbar) + notET events in bins of notET.


pdgid: S030DMP
text:
AABOUD 2017AQ search for WIMP in p p --> h ( gamma gamma) + notET in 36.1 fb**-1 of data. Limits on the visible cross section are also provided. Model dependent limits on spin independent DM - Nucleon cross-section are also presented, which are more stringent than those from direct searches for DM mass smaller than 2.5 GeV.


pdgid: S030DMP
text:
AABOUD 2017BD search for p p -->jet(s) + notET at 13 TeV with 3.2 fb**-1 of data. Limits set for simplified models. Observables corrected for detector effects can be used to constrain other models.


pdgid: S030DMP
text:
AABOUD 2017R, for an axial vector mediator in the s-channel, excludes m(mediator) < 750 -- 1200 GeV for m(DM) < 230 -- 480 GeV, depending on the couplings.


pdgid: S030DMP
text:
AGUILAR-AREVALO 2017A search for DM produced in 8 GeV proton collisions with steel beam dump followed by DM-nucleon scattering in MiniBooNE detector. Limit placed on DM cross section parameter Y < 2E-8 for alpha_{{D}} = 0.5 and for 0.01 < m(DM) < 0.3 GeV.


pdgid: S030DMP
text:
BANERJEE 2017 search for dark photon invisible decay via e N scattering; exclude m(gamma^') < 100 MeV as an explanation of (g_{{mu}}-2) muon anomaly.


pdgid: S030DMP
text:
KHACHATRYAN 2017A search for WIMPs in forward jets + notET channel with 18.5 fb**-1 at 8 TeV; limits set in effective theory model, Fig. 3.


pdgid: S030DMP
text:
KHACHATRYAN 2017F search for H -->invisibles in p p collisions at 7, 8, and 13 TeV; place limits on Higgs portal DM.


pdgid: S030DMP
text:
SIRUNYAN 2017 search for p p --> Z + notET with 2.3 fb**-1 at 13 TeV; no signal seen; limits placed on WIMPs and unparticles.


pdgid: S030DMP
text:
SIRUNYAN 2017AP search for p p --> Z^' --> A h --> h + notET with h --> b bbar or gamma gamma and A --> chi chi with 2.3 fb**-1 at 13 TeV. Limits set in m(Z^') vs. m(A) plane.


pdgid: S030DMP
text:
SIRUNYAN 2017AQ search for p p --> gamma + notET at 13 TeV with 12.9 fb**-1. Limits derived for simplified DM models, effective electroweak-DM interaction and Extra Dimensions models.


pdgid: S030DMP
text:
SIRUNYAN 2017BB search for WIMPs via p p --> t tbar+notET, p p --> b bbar+notET at 13 TeV with 2.2 fb**-1. Limits derived for various simplified models.


pdgid: S030DMP
text:
SIRUNYAN 2017G search for p p --> j + notET with 12.9 fb**-1 at 13 TeV; limits placed on WIMP mass/mediators in DM simplified models.


pdgid: S030DMP
text:
SIRUNYAN 2017U search for WIMPs/unparticles via p p --> Z chi chi, Z --> lepton leptonbar at 13 TeV with 2.3 fb**-1. Limits derived for various simplified models.


pdgid: S030DMP
text:
AABOUD 2016AD place limits on V V X X effective theory via search for hadronic W or Z plus WIMP pair production. See Fig. 5.


pdgid: S030DMP
text:
AAD 2016AF search for V V --> (H --> WIMP pair) + forward jets with 20.3 fb^{-1} at 8 TeV; set limits in Higgs portal model, Fig. 8.


pdgid: S030DMP
text:
AAD 2016AG search for lepton jets with 20.3 fb**-1 of data at 8 TeV; Fig. 13 excludes dark photons around 0.1 -- 1 GeV for kinetic mixing E-6 -- E-2.


pdgid: S030DMP
text:
AAD 2016M search with 20.3 fb**-1 of data at 8 TeV p p collisions; limits placed on EFT model (Fig. 7) and simplified Z^' model (Fig. 6).


pdgid: S030DMP
text:
KHACHATRYAN 2016BZ search for jet(s) + notET in 19.7 fb**-1 at 8 TeV; limits set for variety of simplified models.


pdgid: S030DMP
text:
KHACHATRYAN 2016CA search for WIMPs via jet(s) + notET using razor variable; require mediator scale > 1 TeV for various effective theories.


pdgid: S030DMP
text:
KHACHATRYAN 2016N search for gamma + WIMPs in 19.6 fb**-1 at 8 TeV; limits set on SI and SD WIMP-p scattering in Fig. 3.


pdgid: S030DMP
text:
AAD 2015AS search for events with one or more bottom quark and missing E(T), and also  events with a top quark pair and missing E(T) in p p collisions at Ecm = 8 TeV with  L = 20.3 fb**-1. See their Figs. 5 and 6 for translated limits on X0-nucleon  cross section for m = 1 -- 700 GeV.


pdgid: S030DMP
text:
AAD 2015BH search for events with a jet and missing E(T) in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See their Fig. 12 for translated limits on X0-nucleon cross section for m = 1 -- 1200 GeV.


pdgid: S030DMP
text:
AAD 2015CF search for events with a H0 (--> gamma gamma) and missing E(T) in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See paper for limits on the strength of some contact interactions containing X0 and the Higgs fields.


pdgid: S030DMP
text:
AAD 2015CS search for events with a photon and missing E(T) in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See their Fig. 13 (see also erratum) for translated limits on X0-nucleon cross section for m = 1 -- 1000 GeV.


pdgid: S030DMP
text:
KHACHATRYAN 2015AG search for events with a top quark pair and missing E(T) in p p  collisions at Ecm = 8 TeV with L = 19.7 fb**-1. See their Fig. 8 for translated  limits on X0-nucleon cross section for m = 1 -- 200 GeV.


pdgid: S030DMP
text:
KHACHATRYAN 2015AL search for events with a jet and missing E(T) in p p collisions at  Ecm = 8 TeV with L = 19.7 fb**-1. See their Fig. 5 and Tables 4 -- 6 for translated limits on X0-nucleon cross section for m = 1 -- 1000 GeV.


pdgid: S030DMP
text:
KHACHATRYAN 2015T search for events with a lepton and missing E(T) in p p collisions at Ecm = 8 TeV with L = 19.7 fb**-1. See their Fig. 17 for translated limits on  X0-proton cross section for m = 1 -- 1000 GeV.


pdgid: S030DMP
text:
AAD 2014AI search for events with a W and missing E(T) in p p collisions at  Ecm = 8 TeV with L = 20.3 fb**-1. See their Fig. 4 for translated limits on  X0--nucleon cross section for m = 1 -- 1500 GeV.


pdgid: S030DMP
text:
AAD 2014BK search for hadronically decaying W, Z in association with notET in 20.3 fb**-1 at 8 TeV p p collisions. Fig. 5 presents exclusion results for SI and SD scattering cross section. In addition, cross section limits on the anomalous production of W or Z bosons with large missing transverse momentum are also set in two fiducial regions.


pdgid: S030DMP
text:
AAD 2014K search for events with a Z and missing E(T) in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See their Fig. 5 and 6 for translated limits on X0--nucleon cross section for m = 1 -- 10**3 GeV.


pdgid: S030DMP
text:
AAD 2014O search for Z H0 production with H0 decaying to invisible final states. See their Fig. 4 for translated limits on X0--nucleon cross section for m = 1 -- 60 GeV in Higgs-portal X0 scenario.


pdgid: S030DMP
text:
AAD 2013AD search for events with a jet and missing E(T) in p p collisions at Ecm = 7 TeV with L = 4.7 fb**-1. See their Figs. 5 and 6 for translated limits on X0-nucleon cross section for m = 1 -- 1300 GeV.


pdgid: S030DMP
text:
AAD 2013C search for events with a photon and missing E(T) in p p collisions at  Ecm = 7 TeV with L = 4.6 fb**-1. See their Fig. 3 for translated limits on  X0-nucleon cross section for m = 1 -- 1000 GeV.


pdgid: S030DMP
text:
AALTONEN 2012K search for events with a top quark and missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 7.7 fb**-1. Upper limits on CS(t X0) in the range 0.4 -- 2 pb (95% CL) is given for mass(X0) = 0 -- 150 GeV.


pdgid: S030DMP
text:
AALTONEN 2012M search for events with a jet and missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 6.7 fb**-1. Upper limits on the cross section in the range 2 -- 10 pb (90% CL) is given for mass(X0) = 1 -- 300 GeV. See their Fig. 2 for translated limits on X0-nucleon cross section.


pdgid: S030DMP
text:
CHATRCHYAN 2012AP search for events with a jet and missing E(T) in p p collisions at Ecm = 7 TeV with L = 5.0 fb**-1. See their Fig. 4 for translated limits on X0-nucleon cross section for mass(X0) = 0.1 -- 1000 GeV.


pdgid: S030DMP
text:
CHATRCHYAN 2012T search for events with a photon and missing E(T) in p p collisions at Ecm = 7 TeV with L = 5.0 fb**-1. Upper limits on the cross section in the range 13 -- 15 fb (90% CL) is given for mass(X0) = 1 -- 1000 GeV. See their Fig. 2 for translated limits on X0-nucleon cross section.


pdgid: S015CON
text:
YAMAGATA 1993 used deep sea water at 4000 m since the concentration is enhanced in deep sea due to gravity.


pdgid: S015CON
text:
VERKERK 1992 looked for heavy isotopes in sea water and put a bound on concentration of stable charged massive particle in sea water. The above bound can be translated into into a bound on charged dark matter particle (5E6 GeV), assuming the local density, rho=0.3 GeV/cm**3, and the mean velocity <v>=300 km/s.


pdgid: S015CNM
text:
AFEK 2021 search for millicharged particles bound to matter using an optomechanical device. No signal was observed. Limits placed in the abundance vs. charge plane (Fig. 3). This is translated to the mass versus charge plane by requiring bound states to be stable.


pdgid: S015CNM
text:
JAVORSEK 2001 search for (neutral) SIMPs (strongly interacting massive particles) bound to Au nuclei. Here M is the effective SIMP mass.


pdgid: S015CNM
text:
JAVORSEK 2001B search for (neutral) SIMPs (strongly interacting massive particles) bound to Au and Fe nuclei from various origins with exposures on the earth's surface, in a satellite, heavy ion collisions, etc. Here M is the mass of the anomalous nucleus. See also JAVORSEK 2002.


pdgid: S015NPH
text:
HAYRAPETYAN 2024AO report on search for soft unclustered energy deposits. No signal observed. Limits placed in mediator mass vs. decay temperature plane.


pdgid: S015NPH
text:
ALKHATIB 2021A search for lightly ionizing fractionally charged relics scattering from Ge. No signal observed. Limits plotted in fractional charge f vs. vertical intensity plane for m ~ 5 MeV to 100 TeV.


pdgid: S015NPH
text:
AGUILAR-AREVALO 2020B search for light BSM mediator effect on nu elastic scatter on nuclei; no signal; limits placed in m(mediator) vs. coupling plane for two models of MeV-scale mediators.


pdgid: S015NPH
text:
FEDDERKE 2020 place limits on cosmic relic charged massive particles (CHAMPs) due to their capture and subsequent disruption of old white dwarf stars; limits placed in the m(CHAMP) vs. relic density parameter plane.


pdgid: S015NPH
text:
SIRUNYAN 2020A search for SUSY and LQ production using mT2 or presence of long-lived charged particle; no signal, limits placed in various mass planes for different BSM scenarios and various assumed lifetimes.


pdgid: S015NPH
text:
ALCANTARA 2019 place limits on m(WIMPzilla=X) vs lifetime from upper bound on ultra high energy cosmic rays at Auger experiment: e.g. tau(X) < 4E22 yr for m(X) = E16 GeV.


pdgid: S015NPH
text:
PORAYKO 2018 search for deviations in the residuals of pulsar timing data using PPTA. No signal observed. Limits set on fuzzy DM with 3E-24 < m(DM) <2E-22 eV.


pdgid: S015NPH
text:
AAD 2015AT search for events with a top quark and mssing E(T) in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1.


pdgid: S015NPH
text:
KHACHATRYAN 2015F search for events with a top quark and mssing E(T) in p p collisions at Ecm = 8 TeV with L = 19.7 fb**-1.


pdgid: S015NPH
text:
AALTONEN 2014J examine events with a W and two jets in p pbar collisions at Ecm = 1.96 TeV with L = 8.9 fb**-1. Invariant mass distributions of the two jets are consistent with the Standard Model expectation.


pdgid: S015NPH
text:
AAD 2013C search for events with a photon and missing notET in p p collisions at Ecm = 7 TeV with L = 4.6 fb**-1.


pdgid: S015NPH
text:
AALTONEN 2013I search for events with a photon and missing E(T), where the photon is detected after the expected timing, in p pbar collisions at Ecm = 1.96 TeV with L = 6.3 fb**-1. The data are consistent with the Standard Model expectation.


pdgid: S015NPH
text:
CHATRCHYAN 2013 search for events with an opposite-sign lepton pair, jets, and missing E(T) in p p collisions at Ecm = 7 TeV with L = 4.98 fb**-1.


pdgid: S015NPH
text:
AAD 2012C search for events with a t tbar pair and missing notET in p p collisions at Ecm = 7 TeV with L = 1.04 fb**-1.


pdgid: S015NPH
text:
AALTONEN 2012M search for events with a jet and missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 6.7 fb**-1.


pdgid: S015NPH
text:
CHATRCHYAN 2012AP search for events with a jet and missing E(T) in p p collisions at Ecm = 7 TeV with L = 5.0 fb**-1.


pdgid: S015NPH
text:
CHATRCHYAN 2012Q search for events with a Z, jets, and missing notET in p p collisions at Ecm = 7 TeV with L = 4.98 fb**-1.


pdgid: S015NPH
text:
CHATRCHYAN 2012T search for events with a photon and missing notET in p p collisions at Ecm = 7 TeV with L = 5.0 fb**-1.


pdgid: S015NPH
text:
AAD 2011S search for events with one jet and missing E(T) in p p collisions at Ecm = 7 TeV with L = 33 pb**-1.


pdgid: S015NPH
text:
AALTONEN 2011AF search for high-pT like-sign dileptons in p pbar collisions at Ecm = 1.96 TeV with L = 6.1 fb**-1.


pdgid: S015NPH
text:
CHATRCHYAN 2011C search for events with an opposite-sign lepton pair, jets, and missing E(T) in p p collisions at Ecm = 7 TeV with L = 34 pb**-1.


pdgid: S015NPH
text:
CHATRCHYAN 2011U search for events with one jet and missing E(T) in p p collisions at Ecm = 7 TeV with L = 36 pb**-1.


pdgid: S015NPH
text:
AALTONEN 2010AF search for gamma gamma events with e, mu, tau, or missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 1.1 -- 2.0 fb**-1.


pdgid: S015NPH
text:
AALTONEN 2009AF search for lepton gamma b events with missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 1.9 fb**-1. The observed events are compatible with Standard Model expectation including t tbar gamma production.


pdgid: S015NPH
text:
AALTONEN 2009G search for mu mu mu and mu mu e events with missing E(T) in p pbar collisions at Ecm = 1.96 TeV with L = 976 pb**-1.


pdgid: S015HP
text:
HAYRAPETYAN 2024G search for trijet resonance at CMS with 138 fb**-1 of data at 13 TeV. No signal observed. Limits placed on various models vs mass(resonance).


pdgid: S015HP
text:
TUMASYAN 2023L search for dijet resonance in 4-jet events with 138 fb**-1 fb of data.  There are two events in the tails of the distributions, each with a four-jet mass of 8 TeV and an average dijet mass of 2 TeV, resulting in local and global significances of 3.9 and 1.6 standard deviations, respectively, if interpreted as a signal. Limits set for simplified diquark model.


pdgid: S015HP
text:
AAD 2020AD search for weakly supervised dijet resonance in ATLAS with 139 fb**-1 at 13 TeV; no signal; various limits placed depending on kinematics and production cross section.


pdgid: S015HP
text:
AAD 2020T search for dijet resonance with or without b-jets at 13 TeV and 139 fb**-1; no signal; limits placed in sigma.BF vs mass plane for various BSM models.


pdgid: S015HP
text:
AAD 2020W search for dijet resonance plus lepton with ATLAS at 13 TeV and 139 fb**-1; no signal; limits placed in sigma.BF vs. mass plane for various BSM models.


pdgid: S015HP
text:
SIRUNYAN 2020AI search for dijet resonance in CMS at 13 TeV with 137 fb**-1; no signal; limits set in sigma vs. mass plane for various BSM models.


pdgid: S015HP
text:
AABOUD 2019AJ search for low mass dijet resonance in p p --> gamma X, X --> j j at 13 TeV with 79.8 fb**-1 of data; no signal found; limits placed on Z^' model in coupling vs. m(Z^') plane.


pdgid: S015HP
text:
SIRUNYAN 2019B search for low mass resonance p p --> j A, A --> b bbar at 13 TeV using 35.9 fb**-1; no signal; exclude resonances 50 -- 350 GeV depending on production and decay.


pdgid: S015HP
text:
SIRUNYAN 2019CD search for p p --> Z^' gamma, Z^' --> j j with fat jet (j j); no signal, limits placed in m(Z^') vs. coupling plane for Z^' masses from 10 to 125 GeV.


pdgid: S015HP
text:
AABOUD 2018AD search for new heavy particle Y --> H X --> (b b) + (q q). No signal observed. Limits set on m(Y) vs. m(X) in the ranges of m(Y) in 1 -- 4 TeV and m(X) in 50 -- 1000 GeV.


pdgid: S015HP
text:
AABOUD 2018CK search for SUSY Higgsinos in gauge-mediation via p p --> b b b + notET at 13 TeV using two complementary analyses with 24.3/36.1 fb**-1; no signal is found and Higgsinos with masses between 130 and 230 GeV and between 290 and 880 GeV are excluded at the 95% confidence level.


pdgid: S015HP
text:
AABOUD 2018CL search for p p --> vector-like quarks jets at 13 TeV with 36 fb**-1; no signal seen; limits set on various VLQ scenarios. For pure B --> H b or T --> H t, set the mass limit m > 1010 GeV.


pdgid: S015HP
text:
AABOUD 2018N search for dijet resonance at Atlas with 13 TeV and 29.3 fb**-1; limits set on m(Z^') in the mass range of 450 -- 1800 GeV.


pdgid: S015HP
text:
SIRUNYAN 2018DJ search for p p --> Z Z or W Z --> lepton leptonbar j j resonance at 13 TeV, 35.9 fb**-1; no signal; limits set in the 400 -- 4500 GeV mass range, exclusion of W^' up to 2270 GeV in the HVT model A, and up to 2330 GeV for HVT model B. WED bulk graviton exclusion up to 925 GeV.


pdgid: S015HP
text:
SIRUNYAN 2018DY search for p p --> R R; R --> j j two dijet resonances at 13 TeV 35.9 fb**-1; no signal; limits placed on RPV top-squark pair production.


pdgid: S015HP
text:
KHACHATRYAN 2017W search for dijet resonance in 12.9 fb**-1 data at 13 TeV; see Fig. 2 for limits on axigluons, diquarks, dark matter mediators etc.


pdgid: S015HP
text:
KHACHATRYAN 2017Y search for p p --> (8 -- 10) j in 19.7 fb**-1 at 8 TeV. No signal seen. Limits set on colorons, axigluons, RPV, and SUSY.


pdgid: S015HP
text:
SIRUNYAN 2017F measure p p --> j j angular distribution in 2.6 fb**-1 at 13 TeV; limits set on LEDs and quantum black holes.


pdgid: S015HP
text:
AABOUD 2016 search for resonant dijets including one or two b-jets with 3.2 fb**-1 at 13 TeV; exclude excited b^* quark from 1.1 -- 2.1 TeV; exclude leptophilic Z^' with SM couplings from 1.1 -- 1.5 TeV.


pdgid: S015HP
text:
AAD 2016N search for >=3 jets with 3.6 fb**-1 at 13 TeV; limits placed on micro black holes (Fig. 10) and string balls (Fig. 11).


pdgid: S015HP
text:
AAD 2016S search for high mass jet-jet resonance with 3.6 fb**-1 at 13 TeV; exclude portions of excited quarks, W^', Z^' and contact interaction parameter space.


pdgid: S015HP
text:
KHACHATRYAN 2016K search for dijet resonance in 2.4 fb**-1 data at 13 TeV; see Fig. 3 for limits on axigluons, diquarks etc.


pdgid: S015HP
text:
KHACHATRYAN 2016L use data scouting technique to search for j j resonance on 18.8 fb**-1 of data at 8 TeV. Limits on the coupling of a leptophobic Z^' to quarks are set, improving on the results by other experiments in the mass range between 500 -- 800 GeV.


pdgid: S015HP
text:
AAD 2013D search for dijet resonances in p p collisions at Ecm = 7 TeV with L = 4.8 fb**-1. The observed events are compatible with Standard Model expectation. See their Fig. 6 and Table 2 for limits on resonance cross section in the range m = 1.0 -- 4.0 TeV.


pdgid: S015HP
text:
AALTONEN 2013R search for production of a pair of jet-jet resonances in p pbar collisions at Ecm = 1.96 TeV with L = 6.6 fb**-1. See their Fig. 5 and Tables I, II for cross section limits.


pdgid: S015HP
text:
CHATRCHYAN 2013A search for q q, q g, and g g resonances in p p collisions at Ecm = 7 TeV with L = 4.8 fb**-1. See their Fig. 3 and Table 1 for limits on resonance cross section in the range m = 1.0 -- 4.3 TeV.


pdgid: S015HP
text:
CHATRCHYAN 2013A search for b bbar resonances in p p collisions at Ecm = 7 TeV with L = 4.8 fb**-1. See their Fig. 8 and Table 4 for limits on resonance cross section in the range m = 1.0 -- 4.0 TeV.


pdgid: S015HP
text:
AAD 2012S search for dijet resonances in p p collisions at Ecm = 7 TeV with L = 1.0 fb**-1. See their Fig. 3 and Table 2 for limits on resonance cross section in the range = 0.9 -- 4.0 TeV.


pdgid: S015HP
text:
CHATRCHYAN 2012BL search for t tbar resonances in p p collisions at Ecm = 7 TeV with L = 4.4 fb**-1. See their Fig. 4 for limits on resonance cross section in the range m = 0.5 -- 3.0 TeV.


pdgid: S015HP
text:
AAD 2011AG search for dijet resonances in p p collisions at Ecm = 7 TeV with L = 36 pb**-1. Limits on number of events for m = 0.6 -- 4 TeV are given in their Table 3.


pdgid: S015HP
text:
AALTONEN 2011M find a peak in two jet invariant mass distribution around 140 GeV in W + 2 jet events in p pbar collisions at Ecm = 1.96 TeV with L = 4.3 fb**-1.


pdgid: S015HP
text:
ABAZOV 2011I search for two-jet resonances in W + 2 jet events in p pbar collisions at Ecm = 1.96 TeV with L = 4.3 fb**-1 and give limits sigma< (2.6 -- 1.3) pb (95% CL) for m = 110 -- 170 GeV. The result is incompatible with AALTONEN 2011M.


pdgid: S015HP
text:
AAD 2010 search for narrow dijet resonances in p p collisions at Ecm = 7 TeV with L = 315 nb**-1. Limits on the cross section in the range pb is given for mass() = 0.3 -- 1.7 TeV.


pdgid: S015HP
text:
KHACHATRYAN 2010 search for narrow dijet resonances in p p collisions at Ecm = 7 TeV with L = 2.9 pb**-1. Limits on the cross section in the range 1 -- 300 pb is given for mass() = 0.5 -- 2.6 TeV separately in the final states q q, q g, and g g.


pdgid: S015HP
text:
ABE 1999F search for narrow b bbar resonances in p pbar collisions at Ecm=1.8 TeV. Limits on sigma(p pbar --> X+ anything)*B(X --> b bbar) in the range 3 -- 10**3 pb (95%CL) are given for mass(X)=200 -- 750 GeV. See their Table I.


pdgid: S015HP
text:
ABE 1997G search for narrow dijet resonances in p pbar collisions with 106 pb**-1 of data at Ecm = 1.8 TeV. Limits on sigma(p pbar --> X + anything).B(X --> j j) in the range 10**4 -- 10**-1 pb (95%CL) are given for dijet mass m=200 -- 1150 GeV with both jets having |eta|<2.0 and the dijet system having |cos(theta***)|<0.67. See their Table I for the list of limits. Supersedes ABE 1993G.


pdgid: S015HP
text:
ABE 1993G give cross section times branching ratio into light (d, u, s, c, b) quarks for Gamma = 0.02 M. Their Table II gives limits for M = 200 -- 900 GeV and Gamma = (0.02 -- 0.2) M.


pdgid: S015GAM
text:
AAD 2024AT search for h --> ALPs with ALP --> gamma gamma. No signal observed. Limits placed in BF(h) vs. m(ALP) plane.


pdgid: S015GAM
text:
ALBERT 2018C search for WIMP annihilation in Sun to long-lived, radiatively decaying mediator; no signal; limits set on sigma**SD(chi p) assuming long-lived mediator.


pdgid: S015GAM
text:
KHACHATRYAN 2017D search for new scalar resonance decaying to Z gamma with Z --> e+ e-, mu+ mu- in p p collisions at 8 and 13 TeV; no signal seen.


pdgid: S015GAM
text:
AAD 2016AI search for excited quarks (EQ) and quantum black holes (QBH) in 3.2 fb**-1 at 13 TeV of data; exclude EQ below 4.4 TeV and QBH below 3.8 (6.2) TeV for RS1 (ADD) models. The visible cross section limit was obtained for 5 TeV resonance with sigma_{{G}}/M_{{G}} = 2%.


pdgid: S015GAM
text:
KHACHATRYAN 2016M search for gamma gamma resonance using 19.7 fb**-1 at 8 TeV and 3.3 fb**-1 at 13 Tev; slight excess at 750 GeV noted; limit set on RS graviton.


pdgid: S015GAM
text:
ABBIENDI 2000D associated production limit is for mass(X0)= 90 -- 188 GeV, mass(Y0)=0 at Ecm=189 GeV. See also their Fig. 9.


pdgid: S015GAM
text:
ABBIENDI 2000D pair production limit is for mass(X0) = 45 -- 94 GeV, mass(Y0)=0 at Ecm=189 GeV. See also their Fig. 12.


pdgid: S015GAM
text:
ACKERSTAFF 1997B associated production limit is for mass(X0) = 80 -- 160 GeV, mass(Y0)=0 from 10.0 pb**-1 at Ecm = 161 GeV. See their Fig. 3(a).


pdgid: S015GAM
text:
ACKERSTAFF 1997B pair production limit is for mass(X0) = 40 -- 80 GeV, mass(Y0)=0 from 10.0 pb**-1 at Ecm = 161 GeV. See their Fig. 3(b).


pdgid: S015CS
text:
AAD 2024AE search for heavy vector triplet production with decay to boson pairs. No signal was observed. Limits placed in sigma vs m plane. Limits also placed in various two-dimensional coupling planes (g_{{F}}, g_{{H}}, g_{{{{mathit ell}}}}, g_{{{{mathit ell}}}}(3rd Gen), g_{{q}}, g_{{q}}(3rd Gen), g_{{q}}(1st/2nd Gen)).


pdgid: S015CS
text:
AAD 2024BV search for VBF di-Higgs production with decay to boosted 4b state. No signal observed. Limits placed in mass vs. cross section plane for various simplified models.


pdgid: S015CS
text:
AAD 2024CD search for hadronically-decaying W / Z + MET events from new physics with 140 fb**-1 at 13 TeV. No signal observed. Limits placed on various simplified new physics models.


pdgid: S015CS
text:
AAD 2024E uses a new resonance search technique for two-body decays into any pair of lepton, b, and jet with 140 fb**-1 of data. No signal was observed. Limits placed in sigma vs mass plane for various decay modes.


pdgid: S015CS
text:
AAD 2024S search for quantum black hole (QBH) decay to lepton + jet in 140 fb**-1 of data. No signal observed. Limits placed in sigma.BF vs mass plane for ADD and RS models.


pdgid: S015CS
text:
HAYRAPETYAN 2024AB search for heavy neutral leptons N at CMS with 138 fb**-1 of data. No signal observed. Limits placed in mixing angle vs m(N) plane.


pdgid: S015CS
text:
HAYRAPETYAN 2024AC search for heavy long-lived neutrino N produced in B-decays in 41.6 fb**-1 of data. No signal observed. Limits placed in mixing angle vs m(N) plane.


pdgid: S015CS
text:
HAYRAPETYAN 2024AZ search for various new bosons via production and decay to four muon states with 41.5 and 59.7 fb**-1 of data at 13 TeV. No signal observed. Limits placed usually in mass vs. cross section plane for a variety of new physics simplified models.


pdgid: S015CS
text:
AAD 2023P search in 22 channels for exotica produced in association with h --> gamma gamma in 139  fb**-1 of data. No signal observed. Limits placed on production cross section in various channels.


pdgid: S015CS
text:
TUMASYAN 2023BC search for gamma-jet resonance at CMS with 138 fb**-1 of data. No signal observed. Limits placed on quantum black hole and excited quark models.


pdgid: S015CS
text:
TUMASYAN 2023BF search for p p --> p p + gamma / Z + X search where X is missing particle using CMS-TOTEM with 37.2 fb**-1 of data. No signal observed. Limits placed on sigma vs. m plane.


pdgid: S015CS
text:
TUMASYAN 2022AG search for strongly interacting neutral massive particles via trackless jets with 16.1 fb**-1 at 13 TeV; no signal detected; limits placed in mass vs. cross section plane for various simplified models.


pdgid: S015CS
text:
AAD 2021F search for hard monojet production at ATLAS with 139 **-1 of 13 TeV data. No signal observed. Limits placed on invisible production cross-section recoiling against ISR and interpreted in variety of BSM models.


pdgid: S015CS
text:
AAIJ 2020AL search for dimuon resonance from promptly decaying X particle. No signal detected. Limits placed on m(X) up to 60 GeV depending on mixing in 2HDM.


pdgid: S015CS
text:
SIRUNYAN 2020AY measured Upsilon(1S) pair production cross section and searched for new states decaying into Upsilon(1S) mu+ mu- at CMS with 13 TeV with 35.9 fb**-1. No signal is found and limits are set in sigma.BF vs. mass plane for tetra-b-quarks with masses between 17.5 and 19 GeV and for generic search for narrow resonances with mass between 16.5 and 27 GeV.


pdgid: S015CS
text:
SIRUNYAN 2020Z search for BSM physics via multilepton production with CMS at 13 TeV with 137 fb**-1; no signal is found and limits are set on type-III seesaw and other BSM models.


pdgid: S015CS
text:
AABOUD 2019H searches for di-photon-jet resonance at 13 TeV and 36.7 fb**-1 of data; no signal found and limits placed on sigma.BR vs. mass plane for various simplified models.


pdgid: S015CS
text:
AABOUD 2019V review ATLAS searches for mediator-based DM at 7, 8, and 13 TeV with up to 37 fb**-1 of data; no signal found and limits set for wide variety of simplified models of dark matter.


pdgid: S015CS
text:
SIRUNYAN 2019O search for p p --> gamma notET at 13 TeV with 36.1 fb**-1; no signal found and limits set for various simplified models.


pdgid: S015CS
text:
AABOUD 2018CJ make multichannel search for p p --> V V / lepton lepton / lepton nu, V = W,Z,h at 13 TeV, 36.1 fb**-1; no signal found; limits placed for several BSM models.


pdgid: S015CS
text:
AABOUD 2018CM search for lepton-flavor violating resonance in p p --> e mu / e tau / mu tau at 13 TeV, 36.1 fb**-1; no signal is found and limits placed for various BSM models.


pdgid: S015CS
text:
AAIJ 2018AJ search for prompt and delayed dark photon decay A^' --> mu+ mu- at LHCb detector using 1.6 fb**-1 of p p collisions at 13 TeV; limits on m(A^') vs. kinetic mixing are set.


pdgid: S015CS
text:
BANERJEE 2018 search for dark photon A^'/16.7 MeV boson X at NA64 via e Z --> e Z X (A^'); no signal found and limits set on the X-e- coupling epsilon_{{e}} in the range 1.3E-4<=epsilon_{{e}}<=4.2E-4 excluding part of the allowed parameter space.


pdgid: S015CS
text:
BANERJEE 2018A search for invisibly decaying dark photons in e Z --> e Z A^', A^' -->invisible; no signal found and limits set on mixing for m(A^') < 1 GeV.


pdgid: S015CS
text:
MARSICANO 2018 search for dark photon e+ e- --> A^' (gamma) visible decay in SLAC E137 e beam dump data. No signal observed and limits set in epsilon coupling vs m(A^') plane, see their figure 7.


pdgid: S015CS
text:
SIRUNYAN 2018BB search for high mass dilepton resonance; no signal found and exclude portions of p-space of Z^', KK graviton models.


pdgid: S015CS
text:
SIRUNYAN 2018DA search for p p --> Black Hole, string ball, sphaleron via high multiplicity events at 13 TeV, 35.9 fb**-1; no signal, require e.g. m(BH) > 10.1 TeV.


pdgid: S015CS
text:
SIRUNYAN 2018DD search for p p --> j j deviations in dijet angular distribution. No signal observed. Set limits on large extra dimensions, black holes and DM mediators e.g. m(BH) > 5.9 -- 8.2 TeV.


pdgid: S015CS
text:
SIRUNYAN 2018DR search for dimuon resonance in p p --> b mu mubar at 8 and 13 TeV. Slight excess seen at m(mu mubar) ~ 28 GeV in some channels.


pdgid: S015CS
text:
SIRUNYAN 2018DU search for high mass diphoton resonance in p p --> gamma gamma at 13 TeV using 35.9 fb**-1; no signal; limits placed on RS Graviton, LED, and clockwork.


pdgid: S015CS
text:
SIRUNYAN 2018ED search for p p --> V --> W h; h --> b bbar; W --> lepton nu at 13 TeV with 35.9 fb**-1; no signal; limits set on m(W^') > 2.9 TeV.


pdgid: S015CS
text:
AABOUD 2017B exclude m(W^', Z^') <1.49 -- 2.31 TeV depending on the couplings and W^'/Z^' degeneracy assumptions via W H, Z H search in p p collisions at 13 TeV with 3.2 fb**-1 of data.


pdgid: S015CS
text:
AAIJ 2017BR search for long-lived hidden valley pions from Higgs decay. Limits are set on the signal strength as a function of the mass and lifetime of the long-lived particle in their Fig. 4 and Tab. 4.


pdgid: S015CS
text:
AAD 2016O search for high E(T) lepton + (leptons or jets) with 3.2 fb**-1 at 13 TeV; exclude micro black holes mass < 8 TeV (Fig. 3) for models with two extra dimensions.


pdgid: S015CS
text:
AAD 2016R search for W W, W Z, resonance in 20.3 fb**-1 at 8 TeV data; limits placed on massive RS graviton (Fig. 4).


pdgid: S015CS
text:
KRASZNAHORKAY 2016 report p ^7 ^Li --> ^8 ^Be --> e ebar N 5sigma resonance at 16.7 MeV-- possible evidence for nuclear interference or new light boson. However, such nuclear interference was ruled out already by ZANG 2017.


pdgid: S015CS
text:
LEES 2015E search for long-lived neutral particles produced in e+ e- collisions in the Upsilon region, which decays into e+ e-, mu+ mu-, e+- mu-+, pi+ pi-, K+ K-, or pi+- K-+. See their Fig. 2 for cross section limits.


pdgid: S015CS
text:
ADAMS 1997B search for a hadron-like neutral particle produced in p N interactions, which decays into a rho0 and a weakly interacting massive particle. Upper limits are given for the ratio to K_{{L}} production for the mass range 1.2 -- 5 GeV and lifetime 10**-9 -- 10**-4 s. See also our Light Gluino Section.


pdgid: S015CS
text:
GALLAS 1995 limit is for a weakly interacting neutral particle produced in 800 GeV/c p N interactions decaying with a lifetime of 10**-4 -- 10**-8 s. See their Figs. 8 and 9. Similar limits are obtained for a stable particle with interaction cross section 10**-29 -- 10**-33 cm**2. See Fig. 10.


pdgid: S015CS
text:
AKESSON 1991 limit is from weakly interacting neutral long-lived particles produced in p N reaction at 450 GeV/c performed at CERN SPS. Bourquin-Gaillard formula is used as the production model. The above limit is for tau > 10**-7 s. For tau > 10**-9 s, sigma < 10**-30 cm**-2/nucleon is obtained.


pdgid: S015CS
text:
BADIER 1986 looked for long-lived particles at 300 GeV pi- beam dump. The limit applies for nonstrongly interacting neutral or charged particles with mass >2 GeV. The limit applies for particle modes, mu+ pi-, mu+ mu-, pi+ pi- X, pi+ pi- pi+- etc. See their figure 5 for the contours of limits in the mass-tau plane for each mode.


pdgid: S015CS
text:
GUSTAFSON 1976 is a 300 GeV FNAL experiment looking for heavy (m >2 GeV) long-lived neutral hadrons in the M4 neutral beam. The above typical value is for m = 3 GeV and assumes an interaction cross section of 1 mb. Values as a function of mass and interaction cross section are given in figure 2.


pdgid: S015BD
text:
ANDREEV 2024 search for mu --> mu + E(missing). No signal observed. Limits placed on Z^' models and DM models.


pdgid: S015BD
text:
ABRATENKO 2022A search for LLPs from kaon decay in MicroBooNE absorber; no signal observed; limits placed for heavy neutral leptons (HNLs) and Higgs portal scalars (HPSs) in the MeV mass range.


pdgid: S015BD
text:
ANDREEV 2022A search for new light B-L gauge boson Z^' --> nu nubar in electron beam dump at NA64; no signal observed; limits set in m(Z^') vs coupling plane for m(Z^') ~  E-6 -- 1 GeV.


pdgid: S015BD
text:
ANDREEV 2021 search for new invisibly decaying boson X in e Z --> e Z X at NA64. No signal observed. Limits set in coupling vs. m(X) plane for m(X) ~ 10**-3 to 1 GeV.


pdgid: S015BD
text:
No excess neutral-current events leads to CS(production)*CS(interaction)*acceptance <2.26E-71 cm**4/nucleon**2 (CL = 90%) for light neutrals. Acceptance depends on models (0.1 to 4.E-4).


pdgid: S015EE
text:
ADACHI 2023K search for spin-0 LLP called S in B decays. No signal observed. Limits placed in branching fraction vs. m(S) plane.


pdgid: S015EE
text:
ABLIKIM 2017AA search for dark photon A --> lepton leptonbar at 3.773 GeV with 2.93 fb**-1. Limits are set in epsilon vs m(A) plane.


pdgid: S015EE
text:
ACKERSTAFF 1998P search for pair production of long-lived charged particles at Ecm between 130 and 183 GeV and give limits sigma<(0.05 -- 0.2) pb (95%CL) for spin-0 and spin-1/2 particles with m=45 -- 89.5 GeV, charge 1 and 2/3. The limit is translated to the cross section at Ecm=183 GeV with the s dependence described in the paper. See their Figs. 2 -- 4.


pdgid: S015EE
text:
ABREU 1997D search for pair production of long-lived particles and give limits sigma<(0.4 -- 2.3) pb (95%CL) for various center-of-mass energies Ecm=130 -- 136, 161, and 172 GeV, assuming an almost flat production distribution in cos(theta).


pdgid: S015EE
text:
BARATE 1997K search for pair production of long-lived charged particles at Ecm = 130, 136, 161, and 172 GeV and give limits sigma<(0.2 -- 0.4) pb (95%CL) for spin-0 and spin-1/2 particles with m=45 -- 85 GeV. The limit is translated to the cross section at Ecm=172 GeV with the Ecm dependence described in the paper. See their Figs. 2 and 3 for limits on J and J cases.


pdgid: S015EE
text:
AKERS 1995R is a CERN-LEP experiment with Wcm ~ mass(Z). The limit is for the production of a stable particle in multihadron events normalized to sigma(e+ e- --> hadrons). Constant phase space distribution is assumed. See their Fig. 3 for bounds for Q = +-2/3, +-4/3.


pdgid: S015EE
text:
BUSKULIC 1993C is a CERN-LEP experiment with Wcm = mass(Z). The limit is for a pair or single production of heavy particles with unusual ionization loss in TPC. See their Fig. 5 and Table 1.


pdgid: S015EE
text:
ADACHI 1990C is a KEK-TRISTAN experiment with Wcm = 52 -- 60 GeV. The limit is for pair production of a scalar or spin-1/2 particle. See Figs. 3 and 4.


pdgid: S015EE
text:
ADACHI 1990E is KEK-TRISTAN experiment with Wcm = 52 -- 61.4 GeV. The above limit is for inclusive production cross section normalized to CS(e+ e- --> mu+ mu-).beta(3 - beta**2)/2, where beta = (1 - 4m**2/W(cm)**2)**1/2. See the paper for the assumption about the production mechanism.


pdgid: S015EE
text:
KINOSHITA 1982 is SLAC PEP experiment at Wcm = 29 GeV using lexan and Cr39 plastic sheets sensitive to highly ionizing particles.


pdgid: S015EE
text:
BARTEL 1980 is DESY-PETRA experiment with Wcm = 27-35 GeV. Above limit is for inclusive pair production and ranges between 1.E-1 and 1.E-2 depending on mass and production momentum distributions. (See their figures 9, 10, 11).


pdgid: S015Z
text:
AKERS 1995R give the 95% CL limit sigma(X Xbar)/sigma(mu mu) <1.8E-4 for the pair production of singly- or doubly-charged stable particles. The limit applies for the mass range 40.4 -- 45.6 GeV for X+- and <45.6 GeV for X+-+-. See the paper for bounds for Q = +-2/3, +-4/3.


pdgid: S015DY
text:
BARAK 2024 search for milli-charged particle production in p-graphite collisions using skipper CCDs. No signal was observed. Limits at 95% placed in charge vs. mass plane in a wide range of masses in the MeV range.


pdgid: S015DY
text:
HAYRAPETYAN 2024AD search for emerging dark jets from dark mediator pair production in 138 fb**-1 of data at 13 TeV. No signal observed. Limits placed in the dark tau(pi_{{d}}) vs m(mediator) plane.


pdgid: S015DY
text:
AAD 2023BT search for multi-charged long-lived particles with ATLAS detector using 139 fb**-1. No signal observed. Limits placed on LLP mass vs. charge plane.


pdgid: S015DY
text:
SIRUNYAN 2020N search for LLPs using disappearing track signature at CMS at 13 TeV with 101 fb**-1; no signal; limits placed on long-lived winos and higgsinos from SUSY depending on mass and lifetime: e.g. at 95% CL, for a purely higgsino neurtalino, m(chargino) > 750 (175) GeV for tau = 3 (0.05) ns, and for a purely wino neutralino, m(chargino) > 884 (474) GeV for tau = 3 (0.2) ns.


pdgid: S015DY
text:
AAD 2015BJ use 20.3 fb**-1 of p p collisions at Ecm = 8 TeV. See paper for limits for |Q| = 3, 4, 5, 6.


pdgid: S015DY
text:
CHATRCHYAN 2013AB use 5.0 fb**-1 of p p collisions at Ecm = 7 TeV and 18.8 fb**-1 at Ecm = 8 TeV. See paper for limits for |Q| = 3, 4,..., 8.


pdgid: S015CH
text:
AAD 2024AK search for single top + MET in 140 fb**-1 fb of data. No signal observed. Limits placed in various planes such as sigma vs m(mediator) for assumed simplified models.


pdgid: S015CH
text:
AAD 2024B search for non-resonant jets +MET at sqrt(s) = 13 TeV with 139 fb**-1. No excess observed. Limits placed on dark sector model mediator mass and coupling.


pdgid: S015CH
text:
AAD 2024CM search for new dark mesons decaying to t / b states with 140 fb**-1 at 13 TeV. No signal observed. Limits placed in mass vs. sigma plane for various new physics simplified models.


pdgid: S015CH
text:
AAD 2022G search for single vector-like quark T with T --> t h in all hadronic mode with 139 fb**-1 at 13 TeV; no signal observed; limits placed in mass vs. coupling plane.


pdgid: S015CH
text:
TUMASYAN 2022H search for new states of matter via non-resonant mutilepton production based  on a luminosity of 138 fb**-1; no signal observed; limits placed on vector-like leptons,  leptoquarks, and new fermions from type-III seesaw model.


pdgid: S015CH
text:
SIRUNYAN 2021T perform model unspecific search for deviations from SM with CMS at 13 TeV with 35.9**-1 fb data in numerous signature channels. No deviations from SM found.


pdgid: S015CH
text:
SIRUNYAN 2020C search for four top-quark production with decay to multileptons at CMS at 13 TeV with 137 fb**-1; no signal is found and limits are placed on the Higgs boson oblique parameter in the effective field theory framework (EFT) and the model parameters (tanbeta).


pdgid: S015CH
text:
AABOUD 2019AA search for BSM physics at 13 TeV with 3.2 fb**-1 in >10**5 regions of > 700 event classes; no significant signal found.


pdgid: S015CH
text:
AABOUD 2019Q search for single top+MET events at 13 TeV with 36.1 fb**-1 of data; no signal found and limits set in sigma or coupling vs. mass plane for variety of simplified models including DM and vector-like top quark T.


pdgid: S015CH
text:
AABOUD 2017D search for W W j j, W Z j j in p p collisions at 8 TeV with 3.2 fb**-1; set limits on anomalous couplings.


pdgid: S015CH
text:
AABOUD 2017L search for the pair production of heavy vector-like T quarks in the Z(nu nu )t X final state.


pdgid: S015CH
text:
SIRUNYAN 2017B search for vector-like quark p p --> T X --> t H X in 2.3 fb**-1 at 13 TeV; no signal seen; limits placed.


pdgid: S015CH
text:
SIRUNYAN 2017C search for vector-like quark p p --> T X --> Z + (t or b) in 2.3 fb**-1 at 13 TeV; no signal seen; limits placed.


pdgid: S015CH
text:
SIRUNYAN 2017J search for p p --> X_5/3() X_5/3() --> t W t W with 2.3 fb**-1 at 13 TeV. No signal seen: m(X) > 1020 (990) GeV for RH (LH) new charge 5/3 quark.


pdgid: S015CH
text:
AAIJ 2015BD search for production of long-lived particles in p p collisions at Ecm = 7 and 8 TeV. See their Table 6 for cross section limits.


pdgid: S015CH
text:
AAD 2013AH search for production of long-lived particles with |q|=(2 -- 6)e in p p collisions at Ecm = 7 TeV with 4.4 fb**-1. See their Fig. 8 for cross section limits.


pdgid: S015CH
text:
AAD 2011I search for production of highly ionizing massive particles in p p collisions at Ecm = 7 TeV with L = 3.1 pb**-1. See their Table 5 for similar limits for |q| = 6e and 17e, Table 6 for limits on pair production cross section.


pdgid: S015CH
text:
AALTONEN 2009Z search for long-lived charged particles in p pbar collisions at Ecm = 1.96 TeV with L = 1.0 fb**-1. The limits are on production cross section for a particle of mass above 100 GeV in the region |eta| ~< 0.7, pT> 40 GeV, and 0.4 <beta< 1.0.


pdgid: S015CH
text:
ABAZOV 2009M search for pair production of long-lived charged particles in p pbar collisions at Ecm = 1.96 TeV with L = 1.1 fb**-1. Limit on the cross section of (0.31 -- 0.04) pb (95% CL) is given for the mass range of 60 -- 300 GeV, assuming the kinematics of stau pair production.


pdgid: S015CH
text:
ABE 1992J look for pair production of unit-charged particles which leave detector before decaying. Limit shown here is for m=50 GeV. See their Fig. 5 for different charges and stronger limits for higher mass.


pdgid: S015CH
text:
CARROLL 1978 look for neutral, S = -2 dihyperon resonance in p p --> 2 K+ X. Cross section varies within above limits over mass range and plab = 5.1-5.9 GeV/c.


pdgid: S015CH
text:
LEIPUNER 1973 is an NAL 300 GeV p experiment. Would have detected particles with lifetime greater than 200 ns.


pdgid: S015D
text:
HAYRAPETYAN 2023F search for anomalous top --> leptons decay via effective operators. No signal observed. Limits placed on EFT operators.


pdgid: S015D
text:
BALDIN 1976 is a 70 GeV Serpukhov experiment. Value is per Al nucleus at theta = 0. For other charges in range -0.5 to -3.0, CL = 90% limit is (2.6E-36)/|(charge)| for mass range (2.1-9.4 GeV)*|(charge)|. Assumes stable particle interacting with matter as do antiprotons.


pdgid: S015D
text:
ALBROW 1975 is a CERN ISR experiment with Ecm = 53 GeV. theta = 40 mr. See figure 5 for mass ranges up to 35 GeV.


pdgid: S015D
text:
JOVANOVICH 1975 is a CERN ISR 26+26 and 15+15 GeV p p experiment. Figure 4 covers ranges Q = 1/3 to 2 and m = 3 to 26 GeV. Value is per GeV momentum.


pdgid: S015D
text:
APPEL 1974 is NAL 300 GeV p ^W experiment. Studies forward production of heavy (up to 24 GeV) charged particles with momenta 24-200 GeV (-charge) and 40-150 GeV (+charge). Above typical value is for 75 GeV and is per GeV momentum per nucleon.


pdgid: S015ICH
text:
BERNSTEIN 1988 limits apply at x = 0.2 and p(T) = 0. Mass and lifetime dependence of limits are shown in the regions: m = 1.5-7.5 GeV and tau = 10**-8-2E-6 s. First number is for hadrons; second is for weakly interacting particles.


pdgid: S015ICH
text:
THRON 1985 is FNAL 400 GeV proton experiment. Mass determined from measured velocity and momentum. Limits are for tau >3E-9 s.


pdgid: S015ICH
text:
ARMITAGE 1979 is CERN-ISR experiment at Ecm = 53 GeV. Value is for x = 0.1 and pT = 0.15. Observed particles at m = 1.87 GeV are found all consistent with being antideuterons.


pdgid: S015ICH
text:
BOZZOLI 1979 is CERN-SPS 200 GeV p N experiment. Looks for particle with tau larger than 10**-8 s. See their figure 11-18 for production cross-section upper limits vs mass.


pdgid: S015ICH
text:
CUTTS 1978 is p ^Be experiment at FNAL sensitive to particles of tau >5E-8 s. Value is for -0.3 <x <0 and pT = 0.175.


pdgid: S015ICH
text:
VIDAL 1978 is FNAL 400 GeV proton experiment. Value is for x = 0 and pT = 0. Puts lifetime limit of <5E-8 s on particle in this mass range.


pdgid: S015RPI
text:
NAKAMURA 1989 is KEK experiment with 12 GeV protons on Pt target. The limit applies for mass ~< 1.6 GeV and lifetime ~> 10**-7 s.


pdgid: S015RPI
text:
BUSSIERE 1980 is CERN-SPS experiment with 200-240 GeV protons on Be and Al target. See their figures 6 and 7 for cross-section ratio vs mass.


pdgid: S015CA
text:
AAD 2021X search for LLPs which come to rest in ATLAS detector to deposit energy between  collisions. No signal observed in 111 fb**-1 of data. Limits placed in lifetime vs. mass place  assuming model with gluino hadrons: e.g. m > 1.4 TeV for tau ~ 10**-5 to  10**3 sec.


pdgid: S015CA
text:
ACHARYA 2021 search for dyons (carrying electric and magnetic charge) and monopoles via production and capture in 6.46 fb^{-1} of 13 TeV LHC data. No signal observed. Limits placed in mass vs. magnetic charge plane.


pdgid: S015CA
text:
ALEKSEEV 1976 and ALEKSEEV 1976B are 61-70 GeV p Serpukhov experiment. Cross section is per Pb nucleus.


pdgid: S015XL
text:
AAD 2024AS search for long-lived dark photons (DP) produced from dark sector. No signal observed. Limits placed in portal coupling vs m(DP) plane.


pdgid: S015XL
text:
AAD 2024BN report on ATLAS search for hadronically-decaying long-lived particles that decay in the tracking detector. No signal was observed. Limits placed in ctau vs cross section or branching fraction plane for various simplified new physics models.


pdgid: S015XL
text:
AAD 2024BZ search for long-lived particle decaying to jets in hadronic calorimeter in association with lepton/jet. No signal observed. Limits placed in ctau vs. cross section plane for various simplified new physics models.


pdgid: S015XL
text:
HAYRAPETYAN 2024AI search for long-lived particles (LLPs) using a Muon Detector Shower with a high hit multiplicity in the muon chambers with 138 fb**-1 of data at 13 TeV. No signal was observed. Limits placed in Higgs BF vs. ctau (lifetime) plane.


pdgid: S015XL
text:
HAYRAPETYAN 2024M search for long-lived charginos in SUSY decays with 138 fb**-1 of data at 13 TeV. No signal observed. Limits placed in mass vs mass difference plane for various simplified models.


pdgid: S015XL
text:
HAYRAPETYAN 2024P search for long-lived particles in SUSY models via displaced vertices with 138 fb**-1 of data at 13 TeV. No signal observed. Limits set in split SUSY and gauge mediated SUSY breaking models.


pdgid: S015XL
text:
HAYRAPETYAN 2024S search for long-lived heavy neutral lepton decaying in muon chambers with 138 fb**-1 of data at 13 TeV. No signal observed. Limits placed in mass vs. mixing angle plane.


pdgid: S015XL
text:
HAYRAPETYAN 2024Y search for displaced dimuons in CMS with 36 fb**-1 of data at 13.6 TeV. No signal observed. Limits placed for various models inclduing Abelian dark Higgs and RPV SUSY.


pdgid: S015XL
text:
AAD 2023AM search for long-lived higgsinos from gauge-mediation which decay to Z or H. No signal observed. Limits placed in ctau vs m(chi) plane for various simplified models.


pdgid: S015XL
text:
AAD 2023AR search for long-lived particles via decay to displaced gamma with 139 fb**-1 of data. No signal observed. Limits placed in m vs. tau and BF vs. tau planes for gauge-mediated SUSY model.


pdgid: S015XL
text:
AAD 2023BQ search for displaced dimuon events in ATLAS detector. No signal observed. Limits placed in smuon lifetime vs. mass plane for long-lived smuon model.


pdgid: S015XL
text:
AAD 2023CO search for monopoles and high-electric-charge LLPs in ATLAS with 139 fb**-1 of data. No signal observed. Limits placed in mass vs. charge plane.


pdgid: S015XL
text:
AAD 2023G search for heavy highly ionizing long-lived particles with 139 fb**-1 of data. No signal observed. Limits placed in m vs. tau plane for several SUSY models.


pdgid: S015XL
text:
AAD 2023I search for light long-lived particles decaying to collimated decay products (e.g. dileptons). No signal observed. Limits placed in BF vs. tau plane.


pdgid: S015XL
text:
TUMASYAN 2023AO search for trackless jets from LLP production at CMS. No signal observed. Limits placed for SUSY model with long-lived neutralino in m(chi) vs. ctau plane.


pdgid: S015XL
text:
TUMASYAN 2023G search for LLP decaying to displaced dimuons at CM with 97.6 fb**-1 fb of data. No signal observed. Limits placed in ctau vs. m plane for hidden Abelian Higgs simplified model.


pdgid: S015XL
text:
AAD 2022H search for scalar mediator decay to two LLPs which decay in muon chambers with 139 fb**-1 at 13 TeV; no signal detected; limits placed on various simplified models.


pdgid: S015XL
text:
AAD 2022K search for LLP pair production via scalar mediator with LLP decay in hadron calorimeter; no signal detected; limits placed for various simplified models.


pdgid: S015XL
text:
AAD 2022U search for chargino LLP via disappearing tracks; no signal observed; limits placed in m(chargino) vs lifetime plane for cases of higgsino- or wino-like chargino.


pdgid: S015XL
text:
AAIJ 2022U reports search for LLP production at LHCB with 5.4 fb**-1 at 13 TeV followed by semileptonic decay to muon; no signal detected; limits placed in mass or lifetime vs. cross section plane for several simplified models.


pdgid: S015XL
text:
ACHARYA 2022A report search for monople and HECO production via DY at 8 TeV LHC with 2.2 fb**-1 with MoEDAL detector; no signal detected; limits placed in mass vs. cross section plane for various electric/magnetic charge scenarios.


pdgid: S015XL
text:
TUMASYAN 2022AD search for heavy neutral lepton which decays as LLP to trilepton state with 138 fb**-1 at 13 TeV; no signal detected; limits placed in mass vs. coupling plane.


pdgid: S015XL
text:
TUMASYAN 2022AF search for LLPs via displaced lepton vertices. The analysis is performed with an integrated luminosity of 118 (113) fb**-1 when analyzing the e e (e mu, mu mu) channel; no signal detected; limits placed for a variety of simplified models.


pdgid: S015XL
text:
TUMASYAN 2022M search in 117 fb**-1 of 13 TeV data for Z H production with H --> S S where  S is a LLP; no signal observed; limits placed in decay length vs. branching fraction plane.


pdgid: S015XL
text:
TUMASYAN 2022N search in 101 fb**-1 of 13 TeV data for LLP production via decay to dimuons; no signal observed; limits placed on mass vs. coupling or lifetime for a variety of simplified models.


pdgid: S015XL
text:
AAD 2021AL reports on ATLAS search for long-lived charged particles with 139 fb**-1 at 13 TeV. No signal observed. Limits placed in lifetime vs. mass plane: e.g. for tau(LLP) ~ 0.1 ns, m(selectron) > 720 GeV.


pdgid: S015XL
text:
AAD 2021BA search for long-lived particles from Z H production (H --> b bbar) with 2 displaced vertices in 139 fb**-1 of data at 13 TeV. No signal detected. Limits placed in branching fraction vs. lifetime plane.


pdgid: S015XL
text:
AAIJ 2021V search for p p --> LLP + LLP with LLPe mu nu in the lifetime range between 2 and 50 ps at LHCb with 5.4 fb**-1 at 13 TeV. No signal observed. Limits placed in LLP cross section vs. mass or lifetime plane for m(LLP) ~ 7 to 50 GeV.


pdgid: S015XL
text:
SIRUNYAN 2021AF search for LLPs at CMS via jets with 2 displaced vertices in 140 fb**-1 of data at 13 TeV. No signal observed. Limits placed for RPV SUSY models in which a long-lived neutralino or gluino decays into a multijet final state with top, bottom, and strange quarks.


pdgid: S015XL
text:
SIRUNYAN 2021U search for long-lived particles (LLPs) via displaced jets at CMS with LHC13 and 132 fb**-1. No signal detected. Limits placed on simplified model production of LLP X --> q qbar with sigma < 0.07 fb for m(X) > 500 GeV and ctau ~ 2 to 250 mm.


pdgid: S015XL
text:
TUMASYAN 2021 search for long-lived particles in CMS muon endcap detector in 137 fb**-1 of data at 13 TeV. No signal detected. Limits are placed depending on the branching fraction of Higgs boson to LLP decaying to d d, b b, and tau+ tau-, depending on proper decay length, and LLP masses.


pdgid: S015XL
text:
AAD 2020D search for opposite-sign dileptons originating from long-lived particles in p p collisions at 13 Tev with 32.8 fb**-1; limits placed in squark cross section vs. ctau plane for RPV SUSY.


pdgid: S015XL
text:
AAD 2020J search for scalar boson decay to two long-lived particles; no signal; limits placed in BF vs ctau plane for various mass hypotheses. This search is also combined with other ATLAS displaced-jet searches.


pdgid: S015XL
text:
AAD 2020M search for long-lived top-squarks decay to mu and hadrons; no signal; limits placed in cross section vs. mass and mass vs. lifetime planes.


pdgid: S015XL
text:
AAD 2020P search for long-lived dark photons produced from the decay of a scalar boson, with each dark photon decaying into displaced collimated leptons or light hadrons at 13 TeV with 36 fb**-1; no signal; limits placed in sigma.BF vs. ctau and other planes.


pdgid: S015XL
text:
AAIJ 2020AL search for long-lived X --> mu+ mu- decays in 5.1 fb**-1 of LHCb data at 13 TeV; no signal; limits placed on m(X) up to 3 GeV depending on kinetic mixing.


pdgid: S015XL
text:
BALL 2020 search for long-lived milli-charged particles produced at LHC; limits placed in charge vs. mass plane (Fig. 8).


pdgid: S015XL
text:
AABOUD 2019AE search for long-lived particles via displaced jets using 10.8 fb**-1 or 33.0 fb**-1 data (depending on a trigger) at 13 TeV; no signal found and limits set in branching ratio vs. decay length plane.


pdgid: S015XL
text:
AABOUD 2019AK searches for long-lived particle Z_{{d}} via p p --> Phi --> Z Z_d at 13 TeV with 36.1 fb**-1; no signal found and limits set in sigmaxBR vs. lifetime plane for simplified model.


pdgid: S015XL
text:
AABOUD 2019AM search for Drell-Yan (DY) production of long-lived multi-charge particles at 13 TeV with 36.1 fb**-1 of data; no signal found and exclude 50 GeV < m(LLMCP) < 980 -- 1220 GeV for electric charge |q| = (2 -- 7)e.


pdgid: S015XL
text:
AABOUD 2019AO search for neutral long-lived particles producing displaced jets at 13 TeV with 36.1 fb**-1 of data; no signal found and exclude regions of sigma.BR vs. lifetime plane for various models.


pdgid: S015XL
text:
AABOUD 2019AT search for heavy, charged long-lived particles at 13 TeV with 36.1 fb**-1; no signal found and upper limits set on masses of various hypothetical particles.


pdgid: S015XL
text:
AABOUD 2019G search for long-lived particle with decay to mu+ mu- at 13 TeV with 32.9 fb**-1; no signal found and limits set in combinations of lifetime, mass and coupling planes for various simplified models.


pdgid: S015XL
text:
SIRUNYAN 2019BH search for long-lived SUSY particles via displaced jets at 13 TeV with 35.9 fb**-1; no signal found and limits placed in mass vs lifetime plane for various hypothetical models.


pdgid: S015XL
text:
SIRUNYAN 2019BT search for displaced jet(s)+notET at 13 TeV with 137 fb**-1; no signal found and limits placed in mass vs lifetime plane for gauge mediated SUSY breaking models.


pdgid: S015XL
text:
SIRUNYAN 2019CA search for gluino/squark decay to long-lived neutralino, decay to gamma in GMSB; no signal, limits placed in m(chi) vs. lifetime plane for SPS8 GMSB benchmark point.


pdgid: S015XL
text:
SIRUNYAN 2019Q search for p p --> j + displaced jet via dark quark with 13 TeV at 16.1 fb**-1; no signal found and limits set in mass vs lifetime plane for dark quark/dark pion model.


pdgid: S015XL
text:
SIRUNYAN 2018AW search for very long lived particles (LLPs) decaying hadronically or to mu mubar in CMS detector; none seen/limits set on lifetime vs. cross section.


pdgid: S015XL
text:
AAIJ 2016AR search for long lived particles from H --> X X with displaced X decay vertex using 0.62 fb**-1 at 7 TeV; limits set in Fig. 7.


pdgid: S015XL
text:
KHACHATRYAN 2016BW search for heavy stable charged particles via ToF with 2.5 fb**-1 at 13 TeV; require stable m(gluinoball) > 1610 GeV.


pdgid: S015DCC
text:
RAM 1994 search for a long-lived doubly-charged fermion X++ with mass between mass(N) and mass(N)+mass(pi) and baryon number +1 in the reaction p p --> X++ n. No candidate is found. The limit is for the cross section at 15degree scattering angle at 460 MeV incident energy and applies for tau(X++) >>0.1 mus.


pdgid: S015F
text:
ALEMANNO 2022 search for flux of fractionally charged particles (FCPs) in space; no signal observed; limits set in flux vs charge plane for mass as low as GeV.


pdgid: S015F
text:
CAO 2022 search for superheavy DM decaying to gamma rays; no signal observed; limits placed in mass vs. lifetime plane for m ~ E5 -- E9 GeV for DM decays to b bbar or tau taubar.


pdgid: S015F
text:
ALVIS 2018 search for fractional charged flux of cosmic matter at Majorana demonstrator; no signal observed and limits are set on the flux of lightly ionizing particles for charge as low as e/1000.


pdgid: S015F
text:
SAITO 1990 candidates carry about 450 MeV/nucleon. Cannot be accounted for by conventional backgrounds. Consistent with strange quark matter hypothesis.


pdgid: S015F
text:
MINCER 1985 is high statistics study of calorimeter signals delayed by 20-200 ns. Calibration with AGS beam shows they can be accounted for by rare fluctuations in signals from low-energy hadrons in the shower. Claim that previous delayed signals including BJORNBOE 1968, DARDO 1972, BHAT 1982, SAKUYAMA 1983B below may be due to this fake effect.


pdgid: S015F
text:
SAKUYAMA 1983B analyzed 6000 extended air shower events. Increase of delayed particles and change of lateral distribution above 10**17 eV may indicate production of very heavy parent at top of atmosphere.


pdgid: S015F
text:
BHAT 1982 observed 12 events with delay >2.E-8 s and with more than 40 particles. 1 eV has good hadron shower. However all events are delayed in only one of two detectors in cloud chamber, and could not be due to strongly interacting massive particle.


pdgid: S015F
text:
MARINI 1982 applied PEP-counter for TOF. Above limit is for velocity = 0.54 of light. Limit is inconsistent with YOCK 1980 YOCK 1981 events if isotropic dependence on zenith angle is assumed.


pdgid: S015F
text:
YOCK 1981 saw another 3 events with Q = +-1 and m about 4.5mass(p) as well as 2 events with m >5.3mass(p), Q = +-0.75+-0.05 and m >2.8mass(p), Q = +-0.70+-0.05 and 1 event with m = (9.3+-3.)mass(p), Q = +-0.89+-0.06 as possible heavy candidates.


pdgid: S015FQ
text:
ADRIANI 2015 search for relatively light quark matter with charge Z = 1 -- 8. See their Figs. 2 and 3 for flux upper limits.


pdgid: S015FQ
text:
AMBROSIO 2000B searched for quark matter (``nuclearites'') in the velocity range (10**-5 -- 1) c. The listed limit is for 2E-3 c.


pdgid: S015FQ
text:
ASTONE 1993 searched for quark matter (``nuclearites'') in the velocity range (10**-3 -- 1) c. Their Table 1 gives a compilation of searches for nuclearites.


pdgid: S015FQ
text:
AHLEN 1992 searched for quark matter (``nuclearites''). The bound applies to velocity <2.5E-3 c. See their Fig. 3 for other velocity/c and heavier mass range.


pdgid: S015FQ
text:
LIU 1988 searched for quark matter (``nuclearites'') in the velocity range (2.5E-3 -- 1)c. A less stringent limit of 5.8E-11 applies for (1 -- 2.5)x10**-3c.


pdgid: S015FQ
text:
NAKAMURA 1985 at KEK searched for quark-matter. These might be lumps of strange quark matter with roughly equal numbers of u, d, s quarks. These lumps or nuclearites were assumed to have velocity of (10**-4-10**-3) c.


pdgid: S015FQ
text:
ULLMAN 1981 is sensitive for heavy slow singly charge particle reaching earth with vertical velocity 100-350 km/s.


pdgid: S015BHP
text:
AAD 2015AN search for black hole or string ball formation followed by its decay to multijet  final states, in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See  their Figs. 6 -- 8 for limits.


pdgid: S015BHP
text:
AAD 2014A search for quantum black hole formation followed by its decay to a gamma and a jet, in p p collisions at Ecm = 8 TeV with L = 20 fb**-1. See their Fig. 3 for limits.


pdgid: S015BHP
text:
AAD 2014AL search for quantum black hole formation followed by its decay to a lepton and a jet, in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See their Fig. 2 for limits.


pdgid: S015BHP
text:
AAD 2014C search for microscopic (semiclassical) black hole formation followed by its decay to final states with a lepton and >= 2 (leptons or jets), in p p collisions at Ecm = 8 TeV with L = 20.3 fb**-1. See their Figures 8 -- 11, Tables 7, 8 for limits.


pdgid: S015BHP
text:
AAD 2013D search for quantum black hole formation followed by its decay to two jets, in p p collisions at Ecm = 7 TeV with L = 4.8 fb**-1. See their Fig. 8 and Table 3 for limits.


pdgid: S015BHP
text:
CHATRCHYAN 2013A search for quantum black hole formation followed by its decay to two jets, in p p collisions at Ecm = 7 TeV with L = 5 fb**-1. See their Figs. 5 and 6 for limits.


pdgid: S015BHP
text:
CHATRCHYAN 2013AD search for microscopic (semiclassical) black hole formation followed by its evapolation to multiparticle final states, in multijet (including gamma, lepton) events in p p collisions at Ecm = 8 TeV with L = 12 fb**-1. See their Figs. 5 -- 7 for limits.


pdgid: S015BHP
text:
AAD 2012AK search for microscopic (semiclassical) black hole formation followed by its decay to final states with a lepton and >= 2 (leptons or jets), in p p collisions at Ecm = 7 TeV with L = 1.04 fb**-1. See their Fig. 4 and 5 for limits.


pdgid: S015BHP
text:
CHATRCHYAN 2012W search for microscopic (semiclassical) black hole formation followed by its evapolation to multiparticle final states, in multijet (including gamma, lepton) events in p p collisions at Ecm = 7 TeV with L = 4.7 fb**-1. See their Figs. 5 -- 8 for limits.


pdgid: S015BHP
text:
AAD 2011AG search for quantum black hole formation followed by its decay to two jets, in p p collisions at Ecm = 7 TeV with L = 36 pb**-1. See their Fig. 11 and Table 4 for limits.


