The general relativistic formulation of the problem of magnetically confined mountains on
neutron stars is presented, and the resulting equations are solved numerically, generalizing …

We present analytic solutions of Maxwell equations in the internal and external background
space—time of a slowly rotating magnetized neutron star. The star is considered isolated …

This work presents an implementation of the resistive magnetohydrodynamic equations for a
generic algebraic Ohm's law which includes the effects of finite resistivity within full General …

The hydromagnetic structure of a neutron star accreting symmetrically at both magnetic
poles is calculated as a function of accreted mass, Ma, starting from a polytropic sphere plus …

We study the surface magnetic field fluctuations due to radial oscillations as a viable cause
for the microstructures of the radio pulsar pulse patterns. The electrical conductivity of matter …

We investigate the thermal, magnetic and rotational evolution of isolated neutron stars
assuming that the dipolar magnetic field is confined to the crust. Our treatment, for the first …

Following the general formalism presented by Rezzolla, Ahmedov and Miller,(1) we here
derive analytic solutions of the electromagnetic fields equations in the internal and external …

Recently, a new class of radio transients in the 5 GHz band and with durations of the order of
hours to days, lacking any visible-light counterparts, was detected by Bower and …

An analysis of the role of general relativistic effects on the decay of a neutron star's magnetic
field is presented. At first, a generalized induction equation on an arbitrary static background …

The phenomena of neutrino spin flavour precession in the presence of an extraneous
magnetic field is a repercussion of neutrino magnetic moment which is consociated with the …