Precise measurement of stellar properties through the observation of continuous
gravitational waves from spinning non-axisymmetric neutron stars can shed light onto new …

Detection of continuous gravitational waves from rapidly spinning neutron stars opens up
the possibility of examining their internal physics. We develop a framework that leverages a …

We consider a simulated population of isolated Galactic neutron stars. The rotational
frequency of each neutron star evolves through a combination of electromagnetic and …

Galactic neutron stars are a promising source of gravitational waves in the analysis band of
detectors such as Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo …

Neutron stars are known to contain extremely powerful magnetic fields. Their effect is to
deform the shape of the star, leading to the potential emission of continuous gravitational …

In this paper we model the gravitational wave emission of a freely precessing neutron star.
The aim is to estimate likely source strengths, as a guide for gravitational wave astronomers …

We discuss different ways that neutron stars can generate gravitational waves, describe
recent improvements in modelling the relevant scenarios in the context of improving detector …

Rapidly rotating neutron stars are promising sources of continuous gravitational wave
radiation for the LIGO and Virgo interferometers. The majority of neutron stars in our galaxy …

The gravitational waves emitted by neutron stars carry unique information about their
structure and composition. Direct detection of these gravitational waves, however, is a …

Searches for continuous gravitational waves (GW) from unknown Galactic neutron stars
provide limits on the shapes of neutron stars. A rotating neutron star will produce GW if …