We systematically study the observable properties of dark-matter admixed neutron stars with
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …

The effect of dark matter (DM) on f-mode oscillations in DM admixed neutron stars (NSs) is
investigated in a comprehensive analysis with particular attention to the role of the nuclear …

The fastest and heaviest pulsar, PSR J0952-0607, with a mass of M= 2.35±0.17 M⊙, has
recently been discovered in the disk of the Milky Way Galaxy. In response to this discovery, a …

We investigate the equilibrium structure and radial oscillations of strange quark stars
admixed with fermionic dark matter. For strange quark matter, we employ a stiff equation of …

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 …

Anisotropy in pressure within a star emerges from exotic internal processes. In this study, we
incorporate pressure anisotropy using the Quasi-Local model. Macroscopic properties …

Non-radial oscillations of Neutron Stars (NSs) provide a means to learn important details
regarding their interior composition and equation of state. We consider the effects of Δ …

Neutron stars (NSs) are incredibly versatile for studying various important aspects of high-
energy and compact-object physics. These celestial objects contain extreme matter at …

The σ-cut scheme was recently proposed as a method of stiffening the neutron-star equation
of state (EoS) at high densities without altering its behavior around the nuclear saturation …

This study presents a universal relation for anisotropic neutron stars, called the $ IfC $
relation, which accounts for the local anisotropic pressure using the Quasi-Local (QL) Model …