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Dark matter effects on the properties of neutron stars: compactness and tidal deformability

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arxiv 2403.17024 v1 pith:LERSWLFQ submitted 2024-03-23 nucl-th

Hong-Ming Liu , Jin-Biao Wei , Zeng-Hua Li , G. F. Burgio , H. C. Das , H.-J. Schulze This is my paper · ORCID
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keywords neutronstarsdarkmatterpropertiesadmixedanalyzedcombination
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We systematically study the observable properties of dark-matter admixed neutron stars, employing a realistic nuclear EOS in combination with self-interacting fermionic dark matter respecting constraints on the self-interaction cross section. Deviations from universal relations valid for nucleonic neutron stars are analyzed over the whole parameter space of the model and unequivocal signals for the presence of dark matter in neutron stars are identified.

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Cited by 1 Pith paper

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  1. Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach

    astro-ph.HE 2026-07 conditional novelty 4.0 of 10

    Fermionic dark matter and strong central magnetic fields both reduce neutron-star maximum mass and radius and lower tidal deformability in single-fluid RMF models, remaining compatible with GW/NICER constraints over t...

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