Type Ia supernovae (SNe Ia) are important distance indicators, element factories, cosmic-ray
accelerators, kinetic-energy sources in galaxy evolution, and end points of stellar binary …

In this work we investigate the equilibrium configurations of white dwarfs in a modified
gravity theory, namely, f (R, T) gravity, for which R and T stand for the Ricci scalar and trace …

The question about the origin of the elements is a fascinating one, that scientists have been
trying to answer for the last seven decades. The formation of light elements in the primordial …

The majority of thermonuclear explosions in the Universe seem to proceed in a rather
standardised way, as explosions of carbon-oxygen (CO) white dwarfs in binary systems …

In this work, we investigate the equilibrium configurations of massive white dwarfs (MWD) in
the context of modified gravity, namely\(f (\mathtt {R, L_m})\) gravity, where\(\mathtt {R}\) …

In this paper we compute models for relativistic white dwarfs in the presence of strong
magnetic fields. These models possibly contribute to superluminous SNIa. With an assumed …

The existence of possible massive white dwarfs more than the Chandrasekhar limit (1.45
M⊙, in which M⊙ is mass of the sun) is a challenging topic. In this regard, and motivated by …

We address the issue of stability of recently proposed significantly super-Chandrasekhar
white dwarfs. We present stable solutions of magnetostatic equilibrium models for super …

We explore the effect of modification to Einstein's gravity in white dwarfs for the first time in
the literature, to the best of our knowledge. This leads to significantly sub-and super …

In this work, we study the properties of strongly magnetized white dwarfs (WDs), taking into
account the electron capture and pycnonuclear fusion reactions instabilities. The structure of …