Magnetic fields appear everywhere in the universe. From stars and galaxies, all the way to
galaxy clusters and remote protogalactic clouds, magnetic fields of considerable strength …

General relativity marked the beginning of modern cosmology and it has since been at the
centre of many of the key developments in this field. In the present review, we discuss the …

In this paper we propose the first better than second order accurate method in space and
time for the numerical solution of the resistive relativistic magnetohydrodynamics (RRMHD) …

We estimate here the electrical and Hall conductivity using a quasiparticle approach for
quark matter. We use a Boltzmann kinetic approach in the presence of external magnetic …

We estimate various transport coefficients of hot and dense hadronic matter in the presence
of magnetic field. The estimation is done through solutions of the relativistic Boltzmann …

We have studied the dynamics of an equal-mass magnetized neutron-star binary within a
resistive magnetohydrodynamic (RMHD) approach in which the highly conducting stellar …

We study the gravitational collapse of a magnetized neutron star using a novel numerical
approach able to capture both the dynamics of the star and the behavior of the surrounding …

We estimate the electrical conductivity and the Hall conductivity of a hot and dense hadron
gas using the relaxation time approximation for the solution of the Boltzmann transport …

We formulate hydrodynamic equations for nonsuperfluid multicomponent magnetized
charged relativistic mixtures, taking into account chemical reactions as well as viscosity …

The relativistic fluid is a highly successful model used to describe the dynamics of many-
particle systems moving at high velocities and/or in strong gravity. It takes as input physics …