Now that detection of gravitational-wave signals from the coalescence of extra-galactic
compact binary star mergers has become nearly routine, it is intriguing to consider other …

Abstract The Einstein Telescope (ET), the European project for a third-generation
gravitational-wave detector, has a reference configuration based on a triangular shape …

The birth of gravitational wave astronomy was triggered by the first detection of a signal
produced by the merger of two compact objects (also known as a compact binary …

Superconducting cavities can operate analogously to Weber bar detectors of gravitational
waves, converting mechanical to electromagnetic energy. The significantly reduced …

Seven years after the first direct detection of gravitational waves, from the collision of two
black holes, the field of gravitational wave astronomy is firmly established. A first detection of …

Non-axisymmetrical deformations of the crust on rapidly rotating neutron stars are one of the
main targets of searches for continuous gravitational waves. The maximum ellipticity, or …

Direct detection of gravitational waves has become a powerful new tool of multi-messenger
astrophysics. Apart from short-duration (transient) events, such as the inspirals and mergers …

Continuous gravitational waves are nearly monochromatic signals emitted by asymmetries
in rotating neutron stars. These signals have not yet been detected. Deep all-sky searches …

More than 100 millisecond pulsars (MSPs) have been discovered in radio observations of
gamma-ray sources detected by the Fermi Large Area Telescope (LAT), but hundreds of …

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 …