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 …

Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

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

The thermal evolution of isolated neutron stars is a key element in unravelling their internal
structure and composition and establishing evolutionary connections among different …

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 …

Our previous investigation within the time-dependent nuclear energy-density functional
theory showed that the nuclear superfluids contained inside cold neutron stars could …

The coupled, time-dependent Gross–Pitaevskii and Ginzburg–Landau equations are solved
simultaneously in three dimensions to investigate the equilibrium state and far-from …

We present the first model aimed at understanding how the Meissner effect in a young
neutron star affects its macroscopic magnetic field. In this model, field expulsion occurs on a …

We develop a theoretical framework that allows us to explore the coupled motion of neutron-
superfluid vortices and proton-superconductor flux tubes in a gravitationally collapsed …

Two-band superconductors exhibit a distinct phase characterized by two correlation lengths,
one smaller and the other larger than the magnetic field penetration length. This regime was …