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 …

Context. The presence of magnetic fields in the crust of neutron stars (NSs) causes a non-
spherically symmetric temperature distribution. The strong temperature dependence of the …

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 …

Context. Long-lived, large-scale magnetic field configurations exist in upper main sequence,
white dwarf, and neutron stars. Externally, these fields have a strong dipolar component …

Neutron star magnetic field evolution is mediated through the Hall effect and Ohmic
dissipation in the crust while ambipolar diffusion is taking place in the core. These effects …

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 …

Over the past decade, the numerical modeling of the magnetic field evolution in
astrophysical scenarios has become an increasingly important field. In the crystallized crust …