Affiliation:
1. Niels Bohr Institute
2. University of Copenhagen
3. Institute for Particle Physics Phenomenology
4. Max-Planck-Institut für Kernphysik
Abstract
Ultralight dark matter interacting with sterile neutrinos would modify the evolution and properties of the cosmic neutrino background through active-sterile neutrino mixing. We investigate how such an interaction would induce a redshift dependence in neutrino masses. We highlight that cosmological constraints on the sum of neutrino masses would require reinterpretation due to the effective mass generated by neutrino-dark matter interactions. Furthermore, we present an example where such interactions can alter the mass ordering of neutrinos in the early Universe, compared to what we expect today. We also address the expected changes in the event rates in a PTOLEMY-like experiment, which aims to detect the cosmic neutrino background via neutrino capture and discuss projected constraints.
Published by the American Physical Society
2024
Funder
Carlsbergfondet
Science and Technology Facilities Council
Horizon 2020 Framework Programme
H2020 Marie Sklodowska-Curie Actions
Durham University
Publisher
American Physical Society (APS)