We present a comprehensive study of compact stars admixed with nonself-annihilating self-
interacting fermionic dark matter, delineating the dependence on the nuclear equation of …

Motivated by recent observations of compact binary gravitational wave events reported by
LIGO/Virgo/KAGRA, we review the basics of dark and hybrid stars 1 and examine their …

We explore the presence of self-interacting bosonic dark matter (DM) within neutron stars
(NSs) in light of the latest multimessenger observations of the Neutron Star Interior …

In this work, we study dark matter (DM) admixed strange quark stars exploring the different
possibilities about the nature of the DM and their effects on the macroscopic properties of …

We study the potential of the axion, a, of Quantum Chromodynamics, in the two-flavor color
superconducting phase of cold and dense quark matter. We adopt a Nambu-Jona-Lasinio …

The influence of the dark matter mass (M χ) and the Fermi momentum (k F DM) on the f 0-
mode oscillation frequency, damping time parameter, and tidal deformability of hadronic …

In the context of the f (Q) f(Q) theory of gravity, a spherically symmetric quintessence DE
model in this article is offered. For this reason, f (Q) f(Q) has the formula f (Q)= a Q 2+ Q …

We investigate the structure and the tidal deformability of the color-flavor locked strange
stars admixed with mirror dark matter. Assuming the stars in the GW170817 event have a …

We studied the possible presence of dark matter (DM) in neutron stars (NSs) and the
structural properties of the DM admixed NSs (DMANSs) in one of our recent works. The …

The equation of state (EOS) for neutron stars is modeled using the Relativistic Mean Field
(RMF) approach with a mesonic nonlinear (NL) interaction, a modified sigma cut potential …