Effects of neutrino-ultralight dark matter interaction on the cosmic neutrino background
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
Authors
- Yuber F. Perez-Gonzalez (ORCID: https://orcid.org/0000-0002-2020-7223)
- Pablo Martínez-Miravé (ORCID: https://orcid.org/0000-0001-8649-0546)
- Manibrata Sen (ORCID: https://orcid.org/0000-0001-7948-4332)
Institutions
- University of Copenhagen (DK)
- Durham University (GB)
- Institute of Particle Physics (CA)
- Niels Brock (DK)
- Max Planck Institute for Nuclear Physics (DE)
Publication Details
- Journal
- Physical review. D/Physical review. D.
- Published
- 2024-09-03
- DOI
- https://doi.org/10.1103/physrevd.110.055005
- Citations
- 4
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 2.64
Funders
- European Commission
- Durham University
- Carlsbergfondet
- Horizon 2020 Framework Programme
- Science and Technology Facilities Council
- H2020 Marie Skłodowska-Curie Actions