XTE J1814-338 as a dark matter admixed neutron star

Abstract

The existence of the ultracompact object XTE J1814-338, with an inferred mass and radius of $M$ = 1.21 $\pm$ 0.05 $M_{\odot }$ and R = 7.0 $\pm$ 0.4 km, presents a great challenge for the theory of neutron stars. Within this context, we revisit the theory of dark-matter-admixed neutron stars and infer the physical properties of this compact object, such as the Fermi momentum of dark matter necessary to compress the star at such low radius, its equation of state, speed of sound, and some macroscopic properties, such as the moment of inertia and the dimensionless tidal parameter. We also compare the physical properties of the XTE J1814-338 with other pulsars, such as the canonical 1.4 M${}_{\odot }$, the PSR J0740 + 6620, and the HESS J1731-347.

10 pages, 2 figures, comments are welcome =)

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Cited by in corpus (9)

• Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter
• Bayesian Quantification of Observability and Equation of State of Twin Stars
• Observational Probes of the Neutron Star Equation of State with Hyperons, Bosonic Dark Matter, and Quark Matter
• Confronting recent light compact star observations with color-flavor locked quark matter
• Probing Strange Dark Matter through $f$-mode Oscillations of Neutron Stars with Hyperons and Quark Matter
• Effective Field Theories for Neutron Stars Physics
• Macroscopic properties of the XTE J1814-338 as a dark matter admixed strange star
• Effects of a Brueckner-Hartree-Fock-corrected effective mass on speed of sound, conformality, and observables of dark matter-admixed neutron stars
• XTE J1814-338 as a strange star admixed with bosonic dark matter