The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Simulating the long-term evolution of temperature and magnetic fields in neutron stars is a
major effort in astrophysics, having significant impact in several topics. A detailed …

Buoyancy-restored modes inside neutron stars depend sensitively on both the microphysical
(eg composition and entropy gradients) and macrophysical (eg stellar mass and radius) …

A strong candidate for a source of gravitational waves is a highly magnetized, rapidly
rotating neutron star (magnetar) deformed by internal magnetic stresses. We calculate the …

In this research, we use the generalized quantum multistream model to describe collective
qusiparticle excitations in electron gas with arbitrary degree of degeneracy and relativity …

With neutron star applications in mind, we developed a theory of diffusion in mixtures of
superfluid, strongly interacting Fermi liquids. By employing the Landau theory of Fermi …

We study ambipolar diffusion in strongly magnetized neutron stars, with special focus on the
effects of neutrino reaction rates and the impact of a superfluid/superconducting transition in …

In this paper, we reconsider the problem of magnetic field diffusion in neutron star cores. We
model the star as consisting of a mixture of neutrons, protons and electrons, and allow for …

Context. The chromosphere is a partially ionized layer of the solar atmosphere that mediates
the transition between the photosphere where the gas motion is determined by the gas …