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

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

Hong-Ming Liu , Jin-Biao Wei , Zeng-Hua Li , G. F. Burgio , H. C. Das , H.-J. Schulze This is my paper

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classification nucl-th
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 2 Pith papers

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