Sensitivities for coherent elastic scattering of solar and supernova neutrinos with future NaI(Tl) dark matter search detectors of COSINE-200/1T
arXiv:2210.01386 · doi:10.1016/j.astropartphys.2023.102890
Abstract
We investigate the prospects for measuring the coherent elastic neutrino-nucleus scattering of solar and supernova neutrinos in future NaI(Tl) dark matter detection experiments. Considering the reduced background and improved light yield of the recently developed NaI(Tl) crystals, more than 3 observation sensitivities of the supernova neutrino within the Milky Way are demonstrated. In the case of the solar neutrino, approximately 3 observations are marginal with a 1 ton NaI(Tl) experiment assuming an order of magnitude reduced background, five photoelectron thresholds, and 5-year data exposure.
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- Nonproportionality of NaI(Tl) Scintillation Detector for Dark Matter Search Experiments
- Search for inelastic WIMP-iodine scattering with COSINE-100
- Scintillation characteristics of an undoped CsI crystal at low-temperature for dark matter search
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