Constraining dark matter self-interaction from kinetic heating in neutron stars
hep-ph, astro-ph.GA
Submitted: 2026-04-23
Updated: 2026-09-10
Comments: 21 pages and 6 figures. Latest version matches the published version
Journal ref: Phys. Rev. D 114, 063021 (2026)
DOI: 10.1103/fwrs-w77m
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Dark Matter in the Standard Model?
- Dark Matter through the Higgs portal
- Interaction in the dark sector
- Implications of Two-component Dark Matter Induced by Forbidden Channels and Thermal Freeze-out
- Interaction in the dark sector: a phenomenological approach
- Manifesting hidden dynamics of a sub-component dark matter
- Dark Matter Results From 54-Ton-Day Exposure of PandaX-II Experiment
- Dark Matter Search Results from a One Tonne$\times$Year Exposure of XENON1T
- Dark Matter capture and annihilation on the First Stars: preliminary estimates
- Scattering searches for dark matter in subhalos: neutron stars, cosmic rays, and old rocks
- Astrophysical and Cosmological Probes of Dark Matter
- Impact of galactic distributions in celestial capture of dark matter
- WIMP Annihilation and Cooling of Neutron Stars
- Multiscatter stellar capture of dark matter
- Heating up Neutron Stars with Inelastic Dark Matter
- TASI Lectures on Indirect Detection of Dark Matter
- Indirect Detection of Dark Matter in the Galaxy
- Warming Nuclear Pasta with Dark Matter: Kinetic and Annihilation Heating of Neutron Star Crusts
- Relativistic capture of dark matter by electrons in neutron stars
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