Gravitational wave asteroseismology of dark matter hadronic stars

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

Research output: Contribution to journalArticlepeer-review

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Abstract

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.

Original languageEnglish
Article number083021
JournalPhysical Review D
Volume109
Issue number8
DOIs
StatePublished - 15 Apr 2024

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