Resonant Spin-Flavor Precession of Sterile Neutrinos

Fuente: arXiv
Salvato in:
Dettagli Bibliografici
Autore principale: Wang, Edward
Natura: Preprint
Pubblicazione: 2023
Soggetti:
Accesso online:
Tags: Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
_version_ 1866913650098307072
author Wang, Edward
author_facet Wang, Edward
contents We analyze the impact of resonant conversions mediated by non-vanishing magnetic moments between active neutrinos and a heavy sterile neutrino on the supernova neutrino flux. We present the level-crossing scheme for such a scenario and derive the neutrino fluxes after conversion, paying particular attention to the order in which the resonances occur. We then compute the expected event rates from the neutronization burst of a future supernova at DUNE and Hyper-Kamiokande to derive new constraints on the neutrino magnetic moment. With this, we find a sensitivity down to a few $10^{-15} μ_B$ for a sterile neutrino in the $O(\rm{eV})$ mass range.
format Preprint
id arxiv_https___arxiv_org_abs_2312_03061
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Resonant Spin-Flavor Precession of Sterile Neutrinos
Wang, Edward
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
We analyze the impact of resonant conversions mediated by non-vanishing magnetic moments between active neutrinos and a heavy sterile neutrino on the supernova neutrino flux. We present the level-crossing scheme for such a scenario and derive the neutrino fluxes after conversion, paying particular attention to the order in which the resonances occur. We then compute the expected event rates from the neutronization burst of a future supernova at DUNE and Hyper-Kamiokande to derive new constraints on the neutrino magnetic moment. With this, we find a sensitivity down to a few $10^{-15} μ_B$ for a sterile neutrino in the $O(\rm{eV})$ mass range.
title Resonant Spin-Flavor Precession of Sterile Neutrinos
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
url https://arxiv.org/abs/2312.03061