The interpretation of pulsar rotational glitches, the sudden increase in spin frequency of
neutron stars, is a half-century-old challenge. The common view is that glitches are driven by …

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 …

∼ 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 …

This review focuses on applications of the ideas of superfluidity and superconductivity in
neutron stars in a broader context, ranging from the microphysics of pairing in nucleonic …

We present a statistical study of the glitch population and the behaviour of the glitch activity
across the known population of neutron stars. An unbiased glitch database was put together …

Because of the development of many-body theories of nuclear matter, the long-standing,
open problem of the equation of state (EOS) of dense matter may be understood in the near …

The current interpretation of the observed late time cooling of transiently accreting neutron
stars in low-mass x-ray binaries during quiescence requires the suppression of neutron …

The recent direct observation of gravitational wave event GW170817 and its GRB170817A
signal has opened up a new window to study neutron stars and heralds a new era of …

The crust-core (CC) phase transition of neutron stars is studied within a unified meta-
modeling of the nuclear Equation of State (EoS). The variational equations in the crust are …

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