White dwarfs are a class of stars with unique physical properties. They present many
challenging problems whose solution requires advanced theories of dense matter, state-of …

In this review we discuss self-consistent methods to calculate the global structure of strongly
magnetised neutron stars within the general-relativistic framework. We outline why solutions …

Modified gravity theories can introduce modifications to the Poisson equation in the
Newtonian limit. As a result, we expect to see interesting features of these modifications …

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\(\mathtt {R}\) …

Recent observations of type Ia supernovae (SNe Ia) have discovered a subclass of" super-
Chandrasekhar" SNe Ia (SC SNe Ia) whose high luminosities and low ejecta velocities …

Using an axisymmetric numerical code, we perform an extensive study of the magnetic-field
configurations in nonrotating neutron stars, varying the mass, magnetic-field strength and …

We present two-dimensional hydrodynamic simulations of the accretion-induced collapse
(AIC) of rotating white dwarfs admixed with an extended component of dark matter (DM) …

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 …

The evolution of white dwarfs (WDs) depends crucially on thermal processes. The plasma in
their core can produce neutrinos that escape from the star, thus contributing to the energy …

In this work, we study the effects of magnetic fields on hot white dwarfs. We model their
interior as a nuclei lattice surrounded by a relativistic free Fermi gas of electrons, accounting …