Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105143011> ?p ?o ?g. }
- W3105143011 endingPage "026" @default.
- W3105143011 startingPage "026" @default.
- W3105143011 abstract "We investigate standard and non-standard solar neutrino signals in direct dark matter detection experiments. It is well known that even without new physics, scattering of solar neutrinos on nuclei or electrons is an irreducible background for direct dark matter searches, once these experiments each the ton scale. Here, we entertain the possibility that neutrino interactions are enhanced by new physics, such as new light force carriers (for instance a dark photon) or neutrino magnetic moments. We consider models with only the three standard neutrino flavors, as well as scenarios with extra sterile neutrinos. We find that low-energy neutrino--electron and neutrino--nucleus scattering rates can be enhanced by several orders of magnitude, potentially enough to explain the event excesses observed in CoGeNT and CRESST. We also investigate temporal modulation in these neutrino signals, which can arise from geometric effects, oscillation physics, non-standard neutrino energy loss, and direction-dependent detection efficiencies. We emphasize that, in addition to providing potential explanations for existing signals, models featuring new physics in the neutrino sector can also be very relevant to future dark matter searches, where, on the one hand, they can be probed and constrained, but on the other hand, their signatures could also be confused with dark matter signals." @default.
- W3105143011 created "2020-11-23" @default.
- W3105143011 creator A5049906609 @default.
- W3105143011 creator A5051143862 @default.
- W3105143011 creator A5079054435 @default.
- W3105143011 date "2012-07-11" @default.
- W3105143011 modified "2023-10-13" @default.
- W3105143011 title "Exploring ν signals in dark matter detectors" @default.
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