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• W2145860733 abstract "We study the hydrostatic equilibrium configuration of an admixture of degenerate dark matter and normal nuclear matter by using a general relativistic two-fluid formalism. We consider non- self-annihilating dark matter particles of mass ~ 1 GeV. The mass-radius relations and moments of inertia of these dark-matter admixed neutron stars are investigated and the stability of these stars is demonstrated by performing a radial perturbation analysis. We find a new class of compact stars which consists of a small normal matter core with radius of a few km embedded in a ten-kilometer- sized dark matter halo. These stellar objects may be observed as extraordinarily small neutron stars that are incompatible with realistic nuclear matter models." @default.
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• W2145860733 date "2011-11-04" @default.
• W2145860733 modified "2023-10-15" @default.
• W2145860733 title "Dark-matter admixed neutron stars" @default.
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• W2145860733 doi "https://doi.org/10.1103/physrevd.84.107301" @default.
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