Constraining mass of the WIMP dark matter with the help of Gravitational Waves posterior
arxiv(2022)
摘要
In this work, we explore the likelihood of neutron star admixed with dark matter (DM) as a secondary compact component of GW190814 merger event and constrain the mass of WIMP, with the help of universality relation, and GW170817 posteriors. We have considered a relatively light neutralino, a component of weakly interacting massive particles, as a dark matter candidate which interacts with the baryonic matter of the neutron star (NS) through the exchange of Higgs boson. The baryonic part of the equations-of-state of NS is considered within the relativistic mean-field model with the IOPB-I, G3, and NL3 parameter sets. In efforts to constrain the WIMP mass, we have presumed the DM inside a neutron star core and analyzed its effects on the $M-R$ curves, and $C-\Lambda$ universality relations at different DM masses. With the help of obtained deviation of $C-\Lambda$ curves from the fitted curve when no DM is present, and consequently, the relative shift of MR curves, we constrain the mass of WIMP $M_{DM} \sim 20$ GeV, presuming stiffer equation of state- NL3- to be sacred. The neutron star, described by NL3 EOS, admixed with DM of particle mass $\sim 20$ GeV satisfies the mass and radius range of secondary compact object of GW190814 event, and thus it could be a possible candidate.
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