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Dark matter effects on the properties of neutron stars: compactness and tidal deformability
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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 3 Pith papers
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Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars
First consistent numerical simulations of dark-matter-admixed neutron star mergers show that dark matter cores favor black hole collapse, halos form common envelopes, and standard tidal deformability calculations fail...
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Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach
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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Masquerading hybrid stars with dark matter
Dark matter compression can trigger quark cores in unusually light neutron stars while leaving the mass-radius relation unchanged, producing 'masquerading hybrid stars' and, for light strongly interacting dark matter,...
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