TY - JOUR
T1 - Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
AU - Reno, Mary Hall
AU - Jeong, Yu Seon
AU - Palomares-Ruiz, Sergio
AU - Sarcevic, Ina
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
PY - 2021/4/15
Y1 - 2021/4/15
N2 - While three flavors of “active” neutrinos are consistent with mixing angle results within error bars, there are anomalies may be hints of physics beyond the standard model that can accommodate a fourth mostly “sterile" neutrino species with an eV-scale mass and a mixing angle with active neutrinos of order ?0 ' 0.1. We describe a scenario with eV-scale sterile neutrinos that have self-interactions via a new gauge vector boson, a “secret” mediator f. We show that their production in the early Universe via mixing with active neutrinos is consistent with Big Bang Nucleosynthesis and free-streaming constraints in the Cosmic Microwave Background epoch. For Mf = 4 - 8 keV and sterile neutrino coupling gs = 10-4, we find that resonant interactions of diffuse supernova neutrinos with relic sterile neutrinos in transit to the Earth would cause spectral dips in the neutrino flux. We illustrate the corresponding (anti-)neutrino event distributions as a function of energy in the DUNE (Hyper-Kamiokande) detector.
AB - While three flavors of “active” neutrinos are consistent with mixing angle results within error bars, there are anomalies may be hints of physics beyond the standard model that can accommodate a fourth mostly “sterile" neutrino species with an eV-scale mass and a mixing angle with active neutrinos of order ?0 ' 0.1. We describe a scenario with eV-scale sterile neutrinos that have self-interactions via a new gauge vector boson, a “secret” mediator f. We show that their production in the early Universe via mixing with active neutrinos is consistent with Big Bang Nucleosynthesis and free-streaming constraints in the Cosmic Microwave Background epoch. For Mf = 4 - 8 keV and sterile neutrino coupling gs = 10-4, we find that resonant interactions of diffuse supernova neutrinos with relic sterile neutrinos in transit to the Earth would cause spectral dips in the neutrino flux. We illustrate the corresponding (anti-)neutrino event distributions as a function of energy in the DUNE (Hyper-Kamiokande) detector.
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M3 - Conference article
AN - SCOPUS:85105519275
SN - 1824-8039
VL - 390
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 603
T2 - 40th International Conference on High Energy Physics, ICHEP 2020
Y2 - 28 July 2020 through 6 August 2020
ER -