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Main Authors: Carenza, Pierluca, Lucente, Giuseppe, Mastrototaro, Leonardo, Mirizzi, Alessandro, Serpico, Pasquale Dario
Format: Preprint
Published: 2023
Subjects:
Online Access:https://arxiv.org/abs/2311.00033
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author Carenza, Pierluca
Lucente, Giuseppe
Mastrototaro, Leonardo
Mirizzi, Alessandro
Serpico, Pasquale Dario
author_facet Carenza, Pierluca
Lucente, Giuseppe
Mastrototaro, Leonardo
Mirizzi, Alessandro
Serpico, Pasquale Dario
contents Sterile neutrinos with masses up to $\mathcal{O} (100)$ MeV can be copiously produced in a supernova (SN) core, through the mixing with active neutrinos. In this regard the SN 1987A detection of neutrino events has been used to put constraints on active-sterile neutrino mixing, exploiting the well-known SN cooling argument. We refine the calculation of this limit including neutral current interactions with nucleons, that constitute the dominant channel for sterile neutrino production. We also include, for the first time, the charged current interactions between sterile neutrinos and muons, relevant for the production of sterile neutrinos mixed with muon neutrinos in the SN core. Using the recent modified luminosity criterion, we extend the bounds to the case where sterile states are trapped in the stellar core. Additionally, we study the decays of heavy sterile neutrinos, affecting the SN explosion energy and possibly producing a gamma-ray signal. We also illustrate the complementarity of our new bounds with cosmological bounds and laboratory searches.
format Preprint
id arxiv_https___arxiv_org_abs_2311_00033
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae
Carenza, Pierluca
Lucente, Giuseppe
Mastrototaro, Leonardo
Mirizzi, Alessandro
Serpico, Pasquale Dario
High Energy Physics - Phenomenology
Sterile neutrinos with masses up to $\mathcal{O} (100)$ MeV can be copiously produced in a supernova (SN) core, through the mixing with active neutrinos. In this regard the SN 1987A detection of neutrino events has been used to put constraints on active-sterile neutrino mixing, exploiting the well-known SN cooling argument. We refine the calculation of this limit including neutral current interactions with nucleons, that constitute the dominant channel for sterile neutrino production. We also include, for the first time, the charged current interactions between sterile neutrinos and muons, relevant for the production of sterile neutrinos mixed with muon neutrinos in the SN core. Using the recent modified luminosity criterion, we extend the bounds to the case where sterile states are trapped in the stellar core. Additionally, we study the decays of heavy sterile neutrinos, affecting the SN explosion energy and possibly producing a gamma-ray signal. We also illustrate the complementarity of our new bounds with cosmological bounds and laboratory searches.
title Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2311.00033