Gravitational waves astronomy allows us to study objects and events invisible in
electromagnetic waves. It is crucial to validate the theories and models of the most …

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

Rotating neutron stars that support long-lived, non-axisymmetric deformations known as
mountains have long been considered potential sources of gravitational radiation. However …

Ever since the observation of peculiar overluminous Type Ia supernovae (SNeIa), exploring
possible violations of the canonical Chandrasekhar mass limit (CML) has become a …

A simple cooling model of white dwarf stars is re-analyzed in Palatini f (R) gravity. Modified
gravity affects the white dwarf structures and consequently their ages. We find that the …

After the prediction of many sub-and super-Chandrasekhar (at least a dozen for the latter)
limiting-mass white dwarfs (WDs), hence apparently a peculiar class of WDs, from the …

Over the past several years, there has been enormous interest in massive neutron stars and
white dwarfs due to either their direct or indirect evidence. The recent detection of …

Over the past two decades, the inference of the violation of the Chandrasekhar mass limit of
white dwarfs (WDs) from indirect observation has been a revolutionary discovery in …

We investigate the luminosity suppression and its effect on the mass–radius relation and
cooling evolution of highly magnetized white dwarfs. Based on the effect of magnetic field …

The indirect evidence for at least a dozen massive white dwarfs (WDs) violating the
Chandrasekhar mass limit is considered to be one of the wonderful discoveries in astronomy …