Since the first proof-of-principle experiments over 25 years ago, atom interferometry has
matured to a versatile tool that can be used in fundamental research in particle physics …

The extreme-mass-ratio inspirals (EMRIs) of stellar-mass compact objects into massive
black holes are an important class of source for the future space-based gravitational-wave …

We review potential low-frequency gravitational-wave sources, which are expected to be
detected by Taiji, a Chinese space-based gravitational-wave detector, estimate the detection …

Whether or not the primordial gravitational wave (GW) produced during inflation is
sufficiently strong to be observable, GWs are necessarily produced from the primordial …

We investigate the potential for the LISA space-based interferometer to detect the stochastic
gravitational wave background produced from different mechanisms during inflation …

There are several common conventions in use by the gravitational-wave community to
describe the amplitude of sources and the sensitivity of detectors. These are frequently …

We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate
that two free-falling reference test masses, such as those needed for a space-based …

Gravitational waves (GWs) were observed for the first time in 2015, one century after
Einstein predicted their existence. There is now growing interest to extend the detection …

We consider gravitational wave production by bubble collisions during a cosmological first-
order phase transition. In the literature, such spectra have been estimated by simulating the …

The levitated sensor detector (LSD) is a compact resonant gravitational-wave (GW) detector
based on optically trapped dielectric particles that is under construction. The LSD sensitivity …