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Hoofdauteurs: Parashari, Priyank, Gluscevic, Vera, Zhang, Yue, Bird, Simeon, Ivanov, Mikhail M., He, Adam
Formaat: Preprint
Gepubliceerd in: 2026
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Online toegang:https://arxiv.org/abs/2602.17821
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author Parashari, Priyank
Gluscevic, Vera
Zhang, Yue
Bird, Simeon
Ivanov, Mikhail M.
He, Adam
author_facet Parashari, Priyank
Gluscevic, Vera
Zhang, Yue
Bird, Simeon
Ivanov, Mikhail M.
He, Adam
contents Sterile neutrinos in the keV mass range have long been considered a well-motivated dark matter (DM) candidate. In this work, we explore a sterile neutrino production mechanism through active neutrino self-interactions in the early universe, assuming that they constitute the full DM abundance. We implement a self-consistent treatment of the sterile-neutrino free streaming and the active-neutrino self-interactions on structure formation, which yield a unique scale-dependent modification to the linear matter power spectrum. We then set bounds on this scenario using a combination of the cosmic microwave background and Ly$α$ forest constraints. Specifically, we utilize the two recent likelihoods derived from eBOSS data: (i) an effective field theory (EFT) based full-shape likelihood and (ii) a compressed likelihood obtained from the PRIYA-simulation emulator. We produce some of the most stringent observational constraints to date on sterile neutrino DM, comparable to the bounds from the most stringent laboratory constraints.
format Preprint
id arxiv_https___arxiv_org_abs_2602_17821
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Lyα forest bounds on sterile neutrino production via neutrino self-interactions
Parashari, Priyank
Gluscevic, Vera
Zhang, Yue
Bird, Simeon
Ivanov, Mikhail M.
He, Adam
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
Sterile neutrinos in the keV mass range have long been considered a well-motivated dark matter (DM) candidate. In this work, we explore a sterile neutrino production mechanism through active neutrino self-interactions in the early universe, assuming that they constitute the full DM abundance. We implement a self-consistent treatment of the sterile-neutrino free streaming and the active-neutrino self-interactions on structure formation, which yield a unique scale-dependent modification to the linear matter power spectrum. We then set bounds on this scenario using a combination of the cosmic microwave background and Ly$α$ forest constraints. Specifically, we utilize the two recent likelihoods derived from eBOSS data: (i) an effective field theory (EFT) based full-shape likelihood and (ii) a compressed likelihood obtained from the PRIYA-simulation emulator. We produce some of the most stringent observational constraints to date on sterile neutrino DM, comparable to the bounds from the most stringent laboratory constraints.
title Lyα forest bounds on sterile neutrino production via neutrino self-interactions
topic Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2602.17821