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- W2014209799 abstract "Weakly Interacting Massive Particles (WIMPs) may constitute most of the matter in the Universe. There are intriguing results from DAMA/LIBRA, CoGeNT and CRESST-II, and more recently CDMS-Si suggesting a relatively light dark matter candidate of mass <10 GeV /c 2 . At the same time, experiments using heavy nuclear targets such as CDMS-Ge and XENON detectors suggest that there is no DM candidates with M W >15 GeV /c 2 . We review the existing experiments and the problems associated with light mass WIMP detection. We find that all six experiments considered (DAMA, CoGeNT, CRESST, CDMS-Si, CDMS-Ge, XENON) are consistent if one assumes that the mass of WIMP is lower than expected: 3.4<M W <6.8 GeV /c 2 . This is followed by a discussion of the properties of new detectors, which may enable more reliable detection of low mass WIMPs." @default.
- W2014209799 created "2016-06-24" @default.
- W2014209799 creator A5035784953 @default.
- W2014209799 creator A5039777858 @default.
- W2014209799 date "2013-10-20" @default.
- W2014209799 modified "2023-09-25" @default.
- W2014209799 title "TOWARDS DETECTION OF LOW MASS WIMPs (M<sub><font>WIMP</font></sub><10<font>GeV</font>/c<sup>2</sup>): MINI-REVIEW" @default.
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- W2014209799 doi "https://doi.org/10.1142/s0217751x13300330" @default.
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