2016
DOI: 10.1103/physrevlett.116.071301
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New Results from the Search for Low-Mass Weakly Interacting Massive Particles with the CDMS Low Ionization Threshold Experiment

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Cited by 366 publications
(434 citation statements)
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“…Limits are shown at 90% C.L. For comparison, results from direct detection experiments (LUX [67], PandaX-II [68], XENON [69], superCDMS [70], and CRESST-II [71]) are also shown. The comparison is model dependent and solely valid in the context of this model.…”
Section: A Limits On the Visible Cross Sectionmentioning
confidence: 99%
See 1 more Smart Citation
“…Limits are shown at 90% C.L. For comparison, results from direct detection experiments (LUX [67], PandaX-II [68], XENON [69], superCDMS [70], and CRESST-II [71]) are also shown. The comparison is model dependent and solely valid in the context of this model.…”
Section: A Limits On the Visible Cross Sectionmentioning
confidence: 99%
“…[GeV] The results from this analysis, in which the region inside the contour is excluded, are compared with limits from the LUX [67], PandaX-II [68], XENON [69], superCDMS [70], and CRESST-II [71] experiments. The comparison is model dependent and solely valid in the context of this model, assuming Dirac fermion DM, mixing angle sin θ ¼ 0.3, and the coupling values g q ¼ 1=3 and g χ ¼ 1.…”
Section: A Limits On the Visible Cross Sectionmentioning
confidence: 99%
“…In figure 1, we show the direct detection constraints in the vs. m K plane from experiments LUX [33] with data from 2013 to 2016, PANDAX-II [32], and CRESST-II [31] as well as CDMSlite [30] for low mass DM. Each panel shows choices of g D = e, 0.1, and 0.01, and the dark matter mass fixed to 0.2m K , 0.495m K , 0.6 GeV, or 30 GeV.…”
Section: Jhep06(2017)077mentioning
confidence: 99%
“…The leading direct detection constraints from LUX [33], PANDAX-II [32], and CRESST-II [31], as well as CDMSlite [30], shown in the vs. m K plane for various choices of g D and m χ . We fix m χ = 0.2m K (top left), m χ = 0.495m K (top right), m χ = 0.6 GeV (bottom left), and m χ = 30 GeV (bottom right), to demonstrate the dependence on the dark matter mass.…”
Section: Jhep06(2017)077mentioning
confidence: 99%
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