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

Fuente: arXiv
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Autores principales: Liu, Hong-Ming, Wei, Jin-Biao, Li, Zeng-Hua, Burgio, G. F., Das, H. C., Schulze, H. -J.
Formato: Preprint
Publicado: 2024
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author Liu, Hong-Ming
Wei, Jin-Biao
Li, Zeng-Hua
Burgio, G. F.
Das, H. C.
Schulze, H. -J.
author_facet Liu, Hong-Ming
Wei, Jin-Biao
Li, Zeng-Hua
Burgio, G. F.
Das, H. C.
Schulze, H. -J.
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2403_17024
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Dark matter effects on the properties of neutron stars: compactness and tidal deformability
Liu, Hong-Ming
Wei, Jin-Biao
Li, Zeng-Hua
Burgio, G. F.
Das, H. C.
Schulze, H. -J.
Nuclear Theory
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.
title Dark matter effects on the properties of neutron stars: compactness and tidal deformability
topic Nuclear Theory
url https://arxiv.org/abs/2403.17024