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 …

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 …

General relativity guarantees a unique one-to-one correspondence between static
observables of neutron stars (NSs) accessible by multimessenger astronomy, such as mass …

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 …

We report here on the first results of a systematic monitoring of southern glitching pulsars at
the Argentine Institute of Radioastronomy that started in the year 2019. We detected a major …

The presence of nuclear pasta is expected to modify the transport properties in the mantle of
neutron stars. The non-spherical geometry of the pasta nuclear clusters leads to …

Understanding the average motion of a multitude of superfluid vortices in the interior of a
neutron star is a key ingredient for most theories of pulsar glitches. In this paper, we propose …