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 …

Gravitational waves (GWs) have a great potential to probe cosmology. We review early
universe sources that can lead to cosmological backgrounds of GWs. We begin by …

Abstract The Laser Interferometer Space Antenna (LISA) will open the mHz band of the
gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying …

TianQin is a proposal for a space-borne detector of gravitational waves in the millihertz
frequencies. The experiment relies on a constellation of three drag-free spacecraft orbiting …

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 …

We review detection methods that are currently in use or have been proposed to search for a
stochastic background of gravitational radiation. We consider both Bayesian and frequentist …

We present a data analysis methodology for a model-independent reconstruction of the
spectral shape of a stochastic gravitational wave background with LISA. We improve a …

The Laser Interferometer Space Antenna (LISA) is a planned space-based observatory to
measure gravitational waves in the millihertz frequency band. This frequency band is …

A first order phase transition at the electroweak scale would lead to the production of
gravitational waves that may be observable at upcoming space-based gravitational wave …

We present a Bayesian parameter estimation progress to infer the stellar mass binary black
hole properties by TianQin, LISA, and TianQin+ LISA. Two typical stellar mass black hole …