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 …

Radio pulsars provide us with some of the most stable clocks in the universe. Nevertheless
several pulsars exhibit sudden spin-up events, known as glitches. More than forty years after …

Pulsar glitches are rapid spin-up events that occur in the rotation of neutron stars, providing
a valuable probe into the physics of the interiors of these objects. Long-term monitoring of a …

The 2016 Vela glitch observed by the Mount Pleasant radio telescope provides the first
opportunity to study pulse-to-pulse dynamics of a pulsar glitch, opening up new possibilities …

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 …

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 …

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 …

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 …

Enormous progress has been made on observing stellar magnetism in stars from the main
sequence (particularly thanks to the MiMeS, MAGORI and BOB surveys) through to compact …