New Physics Decaying into Metastable Particles: Impact on Cosmic Neutrinos

We investigate decays of hypothetical unstable new physics particles into metastable species such as muons, pions, or kaons in the early Universe, when temperatures are in the MeV range, and study how they affect cosmic neutrinos. We demonstrate that the nontrivial dynamics of metastables in the plasma alters the impact of the new physics particles on the neutrino population, including the effective number of neutrino degrees of freedom, N_{eff}, modifies neutrino spectral distortions, and may induce asymmetries in neutrino and antineutrino energy distributions. These modifications have important implications for observables such as big bang nucleosynthesis and the cosmic microwave background, especially in light of upcoming cosmic microwave background observations aiming to reach percent-level precision on N_{eff}. We illustrate our findings with a few examples of new physics particles and provide a computational tool available for further exploration.

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Publication Details

Journal
Physical Review Letters
Published
2025-03-24
DOI
https://doi.org/10.1103/physrevlett.134.121001
Citations
8
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
14.96

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article

New Physics Decaying into Metastable Particles: Impact on Cosmic Neutrinos

Thomas Schwetz, Maksym Ovchynnikov, Kensuke Akita, Vsevolod Syvolap et al.
8 citations
Physical Review Letters
Astrophysics and Cosmic Phenomena
14.96
article

New Physics Decaying into Metastable Particles: Impact on Cosmic Neutrinos

Thomas Schwetz, Maksym Ovchynnikov, Kensuke Akita, Vsevolod Syvolap, G. Baur
article en
8 citations

Abstract

We investigate decays of hypothetical unstable new physics particles into metastable species such as muons, pions, or kaons in the early Universe, when temperatures are in the MeV range, and study how they affect cosmic neutrinos. We demonstrate that the nontrivial dynamics of metastables in the plasma alters the impact of the new physics particles on the neutrino population, including the effective number of neutrino degrees of freedom, N_{eff}, modifies neutrino spectral distortions, and may induce asymmetries in neutrino and antineutrino energy distributions. These modifications have important implications for observables such as big bang nucleosynthesis and the cosmic microwave background, especially in light of upcoming cosmic microwave background observations aiming to reach percent-level precision on N_{eff}. We illustrate our findings with a few examples of new physics particles and provide a computational tool available for further exploration.

Physical Review LettersVol. 134(12)
Karlsruhe Institute of Technology (DE), Leiden University (NL), University of Bonn (DE), European Organization for Nuclear Research (CH), The University of Tokyo (JP)
European Commission, Horizon 2020 Framework Programme, Japan Society for the Promotion of Science
Affordable and clean energy
Openalex Percentile: Top 1%
Astrophysics and Cosmic Phenomena
14.96
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