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 …

Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

Continuous gravitational waves (CWs) are quasi-monochromatic signals expected to be
ever-present in the data of gravitational-wave (GW) detectors such as Advanced LIGO (Aasi …

Among the various oscillation modes of neutron stars, f-and g-modes are the most likely to
be ultimately observed in binary neutron star mergers due to their relatively large coupling …

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 …

Magnetars are neutron stars with extremely high magnetic fields (≳ 1014 gauss) that exhibit
various X-ray phenomena such as sporadic subsecond bursts, long-term persistent flux …

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 …

We consider the effects of an attractive, long-range Yukawa interaction between baryons
and dark matter (DM), focusing in particular on temperature and pulsar timing observations …

Pulsars are rotating neutron stars that emit periodic electromagnetic radiation. While pulsars
generally slow down as they lose energy, some also experience glitches: spontaneous …