Gravitational wave asteroseismology of dark matter hadronic stars

César V. Flores, C. H. Lenzi, M. Dutra, O. Lourenço, José D.V. Arbañil

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

6 Citas (Scopus)

Resumen

The influence of the dark matter mass (Mχ) and the Fermi momentum (kFDM) on the f0-mode oscillation frequency, damping time parameter, and tidal deformability of hadronic stars are studied by employing a numerical integration of hydrostatic equilibrium, nonradial oscillation, and tidal deformability equations. The matter inside the hadronic stars follows the NL3∗ equation of state. We obtain that the influence of Mχ and kFDM is observed in the f0-mode, damping tome parameter, and tidal deformability. Finally, the correlation between the tidal deformability of the GW170817 event with Mχ and kFDM are also investigated.

Idioma originalInglés
Número de artículo083021
PublicaciónPhysical Review D
Volumen109
N.º8
DOI
EstadoPublicada - 15 abr. 2024

Huella

Profundice en los temas de investigación de 'Gravitational wave asteroseismology of dark matter hadronic stars'. En conjunto forman una huella única.

Citar esto