Gravitational waves from isolated sources have eluded detection so far. The upper limit of
long-lasting continuous gravitational wave emission can now probe physically motivated …

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 …

Two classes of high-energy sources in our galaxy are believed to host magnetars, ie neutron
stars whose emission results from the dissipation of their magnetic field. The extremely high …

So far, only transient gravitational waves (GWs) produced by catastrophic events of extra-
galactic origin have been detected. However, it is generally believed that there should be …

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 …

It was recently reported that there exists a population of 'glitch candidates' and 'antiglitch
candidates' which are effectively small spin-ups and spin-downs of a neutron star with …

This work explores whether gravitational waves (GWs) from neutron star (NS) mountains can
be detected with current second-generation and future third-generation GW detectors. In …

We study the prospects for the detection of continuous gravitational signals from normal
Galactic neutron stars, ie, nonrecycled stars. We use a synthetic population generated by …

Gravitational waves are expected to be produced from neutron star oscillations associated
with magnetar giant flares and short bursts. We present the results of a search for short …

Observations of short gamma-ray bursts indicate ongoing energy injection following the
prompt emission, with the most likely candidate being the birth of a rapidly rotating, highly …