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 …

∼ 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 …

We report on a timing programme of 74 young pulsars that have been observed by the
Parkes 64-m radio telescope over the past decade. Using modern Bayesian timing …

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 …

PSR J0537–6910 is a young (1–5 kyr) energetic X-ray pulsar, rotating at a spin frequency ν=
62 Hz (Marshall et al. 1998), in the Large Magellanic Cloud at a distance of 49.6 kpc …

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 …

Neutron stars are known to show accelerated spin-up of their rotational frequency called a
glitch. Highly magnetized rotating neutron stars (pulsars) are frequently observed by radio …

Reversible to irreversible (R-IR) transitions arise in numerous periodically driven collectively
interacting systems that, after a certain number of driving cycles, organize into a reversible …

ABSTRACT PSR J0537− 6910, also known as the Big Glitcher, is the most prolific glitching
pulsar known, and its spin-induced pulsations are only detectable in X-ray. We present …

Spinning neutron stars, when observed as pulsars, are seen to undergo occasional spin-up
events known as glitches. Despite several decades of study, the physical mechanisms …