Improved model-dependent corollary analyses after the first six annual cycles of DAMA/LIBRA-phase2

Abstract

Several of the many proposed Dark Matter candidate particles, already investigated with lower exposure and a higher software energy threshold, are further analyzed including the first DAMA/LIBRA--phase2 data release, with an exposure of 1.13 ton $\times$ yr and a lower software energy threshold (1 keV). The cumulative exposure above 2 keV considering also DAMA/NaI and DAMA/LIBRA--phase1 results is now 2.46 ton $\times$ yr. The analysis permits to constraint the parameters' space of the considered candidates restricting their values -- with respect to previous analyses -- thanks to the increase of the exposure and to the lower energy threshold.

arXiv comment48 pages, 33 figures; in press on Nucl. Phys. At. Energy (2019)

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Cited by in corpus (12)

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• GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter
• Direct Detection of Dark Matter -- APPEC Committee Report
• Review on dark matter searches
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• Small scale direct dark matter search experiments