The neutron star properties are generally determined by the equation of state of β-
equilibrated dense matter. In this work, we consider the interaction of fermionic dark matter …

We investigate the impact of the neutron-star matter equation of state on the f-and p 1-mode
oscillations of neutron stars obtained within the Cowling approximation and linearized …

We carry out the study of finite nuclei, infinite nuclear matter, and neutron star properties with
the newly developed relativistic force, the Institute of Physics Bhubaneswar-I (IOPB-I). Using …

Within the relativistic mean-field model, we investigate the properties of dark matter (DM)
admixed neutron stars, considering nonrotating objects made of isotropic matter. We adopt …

In this study, we investigate the impact of weakly interacting massive particles (WIMPs) dark
matter (DM) on C–Λ universal relations, GW170817 posterior, and radial oscillations of …

The impact of anisotropic pressure models in neutron stars (NSs) is increasing their
compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …

We study the dark matter (DM) effects on the nuclear matter (NM) parameters characterizing
the equation of states of super dense neutron-rich nucleonic matter. The observables of the …

We investigate the f-mode oscillation of the dark matter admixed hyperon star within the
relativistic Cowling approximation. The macroscopic properties are calculated with the …

One of the most common assumptions has been made that the pressure inside the star is
isotropic in nature. However, the pressure is locally anisotropic in nature which is a more …

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 …