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Study of Supernova \nu-Nucleus Coherent Scattering Interactions

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arxiv 1110.3536 v3 pith:6UUE5R5E submitted 2011-10-16 astro-ph.HE astro-ph.COastro-ph.GA

classification astro-ph.HEastro-ph.COastro-ph.GA
keywords coherentinteractionsneutrinosscatteringsetupssupernovaavailablebackgrounds
verification ladder T0 review T1 audit T2 compute T3 formal
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Presently, there are several experimental setups dedicated to rare event searches, such as dark matter interactions or double beta decay, in the building or commissioning phases. These experiments often use large mass detectors and have excellent performance in terms of energy resolution, low threshold and extremely low backgrounds. In this paper we show that these setups have the possibility to exploit coherent scattering on nuclei to detect neutrinos from galactic supernova explosions, thus enlarging the number of early detection "observatories" available and helping in the collection of valuable data to perform flavour-independent studies of neutrinos' emission spectra.

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Cited by 1 Pith paper

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  1. Sensitivity study of a sapphire detector using Coherent Elastic Neutrino-Nucleus Scattering process

    hep-ph 2025-02 conditional novelty 5.0 of 10

    Projected sensitivities for the proposed ICNSE sapphire detector show it could constrain new scalar and vector mediator masses at reactor sites, though its neutrino magnetic moment and weak mixing angle reach would be modest.

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