We investigate the peculiar nature of strange stars through an analysis of different quark
models, ie vBag model and CFL model equation of states at different parameter sets, and …

We study consistently the effects of magnetic field on hot and dense matter. In particular, we
look for differences that arise due to assumptions that reproduce the conditions produced in …

We have investigated the structural properties of strange quark stars (SQSs) in a modified
theory of gravity known as massive gravity. In order to obtain the equation of state (EOS) of …

We compute the pressure from first principles within perturbative QCD at finite baryon
density and very high magnetic fields up to two-loops and with physical quark masses. The …

We investigate the structure and radial oscillations of anisotropic compact stars composed of
dark energy, using the vanishing complexity factor formalism within general relativity. This …

A neutron star harbors Script O (10 56) electrons in its core, and almost the same number of
muons, with muon decay prohibited by Pauli blocking. However, as macroscopic properties …

Strongly magnetized neutron stars are popular candidates for producing detectable
electromagnetic and gravitational-wave signals. Gravitational collapses of neutron stars …

Magnetic fields are ubiquitous across different physical systems of current interest; from the
early Universe, compact astrophysical objects and heavy-ion collisions to condensed matter …

We compute the quadrupolar gravitoelectric tidal Love numbers of spherical configurations
made of anisotropic matter. Anisotropies are introduced within the vanishing complexity …

This study investigates the structural properties of strange quark stars (SQS) using a
Quantum Chromodynamics (QCD) perturbative model combined with the latest Particle Data …