Neutron stars and quark stars are ideal laboratories to study fundamental physics at supra
nuclear densities and strong gravitational fields. Astrophysical observables, however …

Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …

We investigate the properties of anisotropic, spherically symmetric compact stars, especially
neutron stars (NSs) and strange quark stars (SQSs), made of strongly magnetized matter …

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars
are unique cosmic laboratories for probing the properties of matter under extreme conditions …

With the doors beginning to swing open on the new gravitational wave astronomy, this
review provides an up-to-date survey of the most important physical mechanisms that could …

Motivated by the recent suggestions that very massive pulsar (PSR J0952− 0607) and very
light compact object (HESS J1731− 347) exist, in this article, we revisit the possibility of such …

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 …

We present the implementation of a two-moment-based general-relativistic multigroup
radiation transport module in the G eneral-relativistic mu ltigrid nu merical (Gmunu) code. On …

One of the main challenges in the numerical modeling of binary neutron-star mergers are
long-term simulations of the postmerger remnant over timescales of the order of seconds …

We present herein a new class of singularity-free interior solutions to describe realistic
anisotropic compact stellar objects with spherically symmetric matter distribution. A specific …