Signatures of bulk neutrinos in the early Universe

Neutrino masses and quantum gravity are strong reasons to extend the standard model of particle physics. A large extra dimension can be motivated by quantum gravity and can explain the small neutrino masses with new singlet states that propagate in the bulk. In such a case, a Kaluza-Klein tower of sterile neutrinos emerges. We revisit constraints on towers of sterile neutrinos that come from cosmological observables such as the effective number of noninteracting relativistic species and the dark matter density. These limits generically rule out micron-sized extra dimensions. We explore the weakening of these constraints to accommodate an extra dimension close to the micron size by assuming that the Universe is reheated after inflation to a low temperature. We discuss how such a possibility can be distinguished in the event of a positive signal in a cosmological observable. Published by the American Physical Society 2024

Authors

Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-10-03
DOI
https://doi.org/10.1103/physrevd.110.083507
Citations
4
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
1.33

Funders

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article

Signatures of bulk neutrinos in the early Universe

M. Shamma, David McKeen, John N. Ng
4 citations
Physical review. D/Physical review. D.
Cosmology and Gravitation Theories
1.33
article

Signatures of bulk neutrinos in the early Universe

M. Shamma, David McKeen, John N. Ng
article en
4 citations

Abstract

Neutrino masses and quantum gravity are strong reasons to extend the standard model of particle physics. A large extra dimension can be motivated by quantum gravity and can explain the small neutrino masses with new singlet states that propagate in the bulk. In such a case, a Kaluza-Klein tower of sterile neutrinos emerges. We revisit constraints on towers of sterile neutrinos that come from cosmological observables such as the effective number of noninteracting relativistic species and the dark matter density. These limits generically rule out micron-sized extra dimensions. We explore the weakening of these constraints to accommodate an extra dimension close to the micron size by assuming that the Universe is reheated after inflation to a low temperature. We discuss how such a possibility can be distinguished in the event of a positive signal in a cosmological observable. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(8)
TRIUMF, Natural Sciences and Engineering Research Council of Canada, National Research Council Canada
Openalex Percentile: Top 19%
Cosmology and Gravitation Theories
1.33
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