2019
DOI: 10.1016/j.nuclphysb.2019.114678
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Constraints on dark matter interactions from the first results of DarkSide-50

Abstract: In an extended effective operator framework of isospin violating interactions with light mediators, we investigate the compatibility of the candidate signal of the CDMS-II-Si with the latest constraints from DarkSide-50 and XENON-1T, etc. We show that the constraints from DarkSide-50 which utilizes Argon as the target is complementary to that from XENON-1T which utilizes Xenon. Combining the results of the two experiments, we find that for isospin violating interaction with light mediator there is no parameter… Show more

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Cited by 5 publications
(5 citation statements)
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“…They have also been key for neutrinos. In the former case, Xe [1][2][3] and Ar [4,5] are each used by distinct large collaborations, and used both to search for continuous spectra, such as the approximate falling exponential expected from the traditional weakly interacting massive particle (WIMP) [6], or monoenergetic peaks expected from dark photons or bosonic super-WIMPs [7]. In the latter case, argon is used in long-and short-baseline oscillation studies [8,9] and xenon in the search for neutrinoless double-beta decay, as either a liquid [10] or a gas [11].…”
Section: Introductionmentioning
confidence: 97%
“…They have also been key for neutrinos. In the former case, Xe [1][2][3] and Ar [4,5] are each used by distinct large collaborations, and used both to search for continuous spectra, such as the approximate falling exponential expected from the traditional weakly interacting massive particle (WIMP) [6], or monoenergetic peaks expected from dark photons or bosonic super-WIMPs [7]. In the latter case, argon is used in long-and short-baseline oscillation studies [8,9] and xenon in the search for neutrinoless double-beta decay, as either a liquid [10] or a gas [11].…”
Section: Introductionmentioning
confidence: 97%
“…This gives different behavior and constraints compared to the previous analysis assuming a single kind of interaction. In this study, we give the realization of the up-scattered DM by cosmic rays of a vector-mediation [9] and complements the existing constraints on this model [14][15][16][17][18][19][20][21][22][23].…”
Section: Introductionmentioning
confidence: 86%
“…At low DM masses, CRESST-III [132], CDMS [133], CDEX [134], and DarkSide [135] provide more stringent constraints, see e.g. the analysis in [18,20,136]. Alternatively the Migdal effect can be exploited [137][138][139][140].…”
Section: B Direct Detectionmentioning
confidence: 99%