Constraining dark matter self-interaction from kinetic heating in neutron stars

arXiv:2604.21652 · hep-ph, astro-ph.GA · Submitted 2026-04-23 · Read on arXiv

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/

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