Neutron stars are natural physical laboratories allowing us to study a plethora of
phenomena in extreme conditions. In particular, these compact objects can have very strong …

Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …

Initial distributions of pulsar periods and magnetic fields are essential components of
multiple modern astrophysical models. Not enough work has been done to properly …

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 …

The long-term evolution of the internal, strong magnetic fields of neutron stars needs a
specific numerical modelling. The diversity of the observed phenomenology of neutron stars …

We perform the first 3D fully coupled magneto-thermal simulations of neutron stars
(including the most realistic background structure and microphysical ingredients so far) …

X-ray emission from the surface of isolated neutron stars (NSs) has been now observed in a
variety of sources. The ubiquitous presence of pulsations clearly indicates that thermal …

Off-centred dipole configurations have been suggested to explain different phenomena in
neutron stars, such as natal kicks, irregularities in polarization of radio pulsars and …

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 …

Neutron stars cool down during their lifetime through the combination of neutrino emission
from the interior and photon cooling from the surface. Strongly magnetized neutron stars …