Abstract
AbstractIn this paper we explore interactions between neutrinos and dark matter. In particular, we study how the propagation of astrophysical neutrinos can be modified by computing the most general potential generated by the galactic DM background. We use on-shell techniques to compute this potential in a completely model independent way and obtain an expression valid for any dark matter mass and spin. Afterwards, we use this expression to analyse under what circumstances such potential can be important at the phenomenological level, and we find that under some assumptions only ultra light scalar dark matter could be of any relevance to oscillation experiments.
Funder
Fundação de Amparo à Pesquisa do Estado de São Paulo
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference61 articles.
1. IceCube Collaboration, First observation of PeV-energy neutrinos with IceCube. Phys. Rev. Lett. 111, 021103 (2013). arXiv:1304.5356
2. A. Olivares-Del Campo, C. Bœhm, S. Palomares-Ruiz, S. Pascoli, Dark matter-neutrino interactions through the lens of their cosmological implications. Phys. Rev. D 97, 075039 (2018). arXiv:1711.05283
3. C. Boehm, A. Olivares-Del Campo, S. Palomares-Ruiz, S. Pascoli, Phenomenology of a neutrino-DM coupling: the scalar case, in Prospects in Neutrino Physics, 5 (2017). arXiv:1705.03692
4. M. Blennow, E. Fernandez-Martinez, A. Olivares-Del Campo, S. Pascoli, S. Rosauro-Alcaraz, A.V. Titov, Neutrino portals to dark matter. Eur. Phys. J. C 79, 555 (2019). arXiv:1903.00006
5. C. Guépin, R. Aloisio, L.A. Anchordoqui, A. Cummings, J.F. Krizmanic, A.V. Olinto et al., Indirect dark matter searches at ultrahigh energy neutrino detectors. Phys. Rev. D 104, 083002 (2021). arXiv:2106.04446
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