Role of Sterile Neutrino Warm Dark Matter in Rhenium and Tritium Beta Decays
H. J. de Vega, O. Moreno, E. Moya de Guerra, M. Ramon Medrano, N., Sanchez

TL;DR
This paper investigates how keV-scale sterile neutrinos, as dark matter candidates, could be detected through small spectral features in Rhenium and Tritium beta decay experiments, offering a new method to identify their presence.
Contribution
It provides a detailed calculation of sterile neutrino effects on beta decay spectra and assesses the potential for detection in current experiments like MARE and KATRIN.
Findings
Sterile neutrino signatures could appear as small kinks in beta spectra.
The energy region for detection is distinct from active neutrino mass measurements.
Current experiments may have the sensitivity to observe these sterile neutrino effects.
Abstract
Sterile neutrinos with mass in the range of one to a few keV are important as extensions of the Standard Model of particle physics and are serious dark matter (DM) candidates. This DM mass scale (warm DM) is in agreement with both cosmological and galactic observations. We study the role of a keV sterile neutrino through its mixing with a light active neutrino in Rhenium 187 and Tritium beta decays. We pinpoint the energy spectrum of the beta particle, 0 < T_e < (Q_{beta} - m_s), as the region where a sterile neutrino could be detected and where its mass m_s could be measured. This energy region is at least 1 keV away rom the region suitable to measure the mass of the light active neutrino, located near the endpoint Q_{beta} . The emission of a keV sterile neutrino in a beta decay could show up as a small kink in the spectrum of the emitted beta particle. With this in view, we perform a…
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