∼ 6% of all known pulsars have been observed to exhibit sudden spin-up events, known as
glitches. For more than fifty years, these phenomena have played an important role in …

Radio pulsars show remarkable clock-like stability, which make them useful astronomy tools
in experiments to test equation of state of neutron stars and detecting gravitational waves …

Motivated by a recent report by Biwas and Bose (Phys Rev D 99: 104002, 2019) that the
observations of GW170817 to constrain the extent of pressure anisotropy in neutron stars …

Calculations of the effects of band structure on the neutron superfluid density in the crust of
neutron stars made under the assumption that the effects of pairing are small [N. Chamel …

As mature neutron stars are cold (on the relevant temperature scale), one has to carefully
consider the state of matter in their interior. The outer kilometre or so is expected to freeze to …

Neutron stars, the compact stellar remnants of core-collapse supernova explosions, are
unique cosmic laboratories for exploring novel phases of matter under extreme conditions …

ABSTRACT PSR J1048 5832 (B1046 58) is a Vela-like pulsar that has exhibited multiple
glitch events. In this study, we analyse the timing data spanning nearly 16 yr, acquired from …

The D1 family of parametrizations of the Gogny interaction commonly suffers from a rather
soft neutron matter equation of state that leads to maximal masses of neutron stars well …

Neutron stars are unique cosmic laboratories in which fundamental physics can be probed
in extreme conditions not accessible to terrestrial experiments. In particular, the precise …

The presence of superfluid phases in the interior of a neutron star affects its dynamics, as it
allows for neutrons to flow relative to the non-superfluid (normal) components of the star with …