Ly alpha forest bounds on sterile neutrino production via neutrino self-interactions
astro-ph.CO, hep-ph
Submitted: 2026-02-19
Updated: 2026-09-15
Comments: 13 pages, 7 figures; Matches the version accepted in Phys. Rev. D
DOI: 10.1103/s1gj-d111
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A History of Dark Matter
- Dark Matter
- Planck 2018 results. VI. Cosmological parameters
- Sterile neutrinos in cosmology
- Constraining Sterile Neutrino Warm Dark Matter with Chandra Observations of the Andromeda Galaxy
- Sterile neutrino dark matter bounds from galaxies of the Local Group
- (Almost) Closing the $\nu$MSM Sterile Neutrino Dark Matter Window with NuSTAR
- The dark matter interpretation of the 3.5-keV line is inconsistent with blank-sky observations
- Constraints on Dark Matter Microphysics from the Milky Way Satellite Population
- A lower bound on the mass of Dark Matter particles
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- Lyman-alpha Forests cool Warm Dark Matter
- Properties of Resonantly Produced Sterile Neutrino Dark Matter Subhalos
- Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100
- New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-$\alpha$ forest data
- Milky Way Satellite Census. III. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies
- Dark Matter Constraints from a Unified Analysis of Strong Gravitational Lenses and Milky Way Satellite Galaxies
- New Constraints on Warm Dark Matter from the Lyman-$\alpha$ Forest Power Spectrum
- Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
- Can Neutrino Self-interactions Save Sterile Neutrino Dark Matter?
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