Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …

The collection of individually resolvable gravitational wave (GW) events makes up a tiny
fraction of all GW signals that reach our detectors, while most lie below the confusion limit …

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

We investigate the sensitivity of the Laser Interferometer Space Antenna (LISA) to the
anisotropies of the Stochastic Gravitational Wave Background (SGWB). We first discuss the …

The formation of merging binary black holes can occur through multiple astrophysical
channels such as, eg, isolated binary evolution and dynamical formation or, alternatively …

The stochastic gravitational wave background (SGWB) offers a new opportunity to observe
signals of primordial features from inflationary models. We study their detectability with future …

Primordial non-Gaussianity encodes vital information of the physics of the early universe,
particularly during the inflationary epoch. To explore the local-type primordial non …

It has been a half-decade since the first direct detection of gravitational waves, which
signifies the coming of the era of the gravitational-wave astronomy and gravitational-wave …

Gravitational radiation offers a unique possibility to study the large-scale structure of the
Universe, gravitational wave sources and propagation in a completely novel way. Given that …

The circular polarization of gravitational waves is a powerful observable to test parity
violation in gravity and to distinguish between the primordial or the astrophysical origin of …