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Dark matter effects on the properties of neutron stars: optical radii

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arxiv 2307.11313 v1 pith:2SM6DY4K submitted 2023-07-21 nucl-th

Hong-Ming Liu , Jin-Biao Wei , Zeng-Hua Li , G. F. Burgio , H.-J. Schulze This is my paper · ORCID
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keywords darkmatterneutronstarseffectsmodelpropertiesradii
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We study the effects of dark matter on the properties of neutron stars by employing a DM-admixed model. The Brueckner-Hartree-Fock theory with realistic three-body forces and a generic bosonic self-interacting dark matter model describe the equations of state for nuclear matter and DM, respectively. We study the complete set of stable dark neutron stars and in particular the observable radii of these objects. A rich variety of stellar configurations is found and discussed in detail.

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  1. Supernova Remnants with Mirror Dark Matter and Hyperons

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Mirror dark matter inside proto-neutron stars reduces maximum mass, radius, and tidal deformability while heating the remnant and raising the speed of sound.

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