Equal-arm detectors of gravitational radiation allow phase measurements many orders of
magnitude below the intrinsic phase stability of the laser injecting light into their arms. This is …

This article reviews the present status of the technology and instrumentation for the joint
ESA/NASA gravitational wave detector LISA. It briefly describes the measurement principle …

We develop a tool for the analysis of stochastic gravitational wave backgrounds from
cosmological first-order phase transitions with LISA: we initiate a template databank for …

The detection of the cosmic microwave background radiation (CMB) was one of the most
important cosmological discoveries of the last century. With the development of …

We propose two distinct atom interferometer gravitational wave detectors, one terrestrial and
another satellite based, utilizing the core technology of the Stanford 10 m atom …

Various scenarios of cosmic inflation enhance the amplitude of the stochastic gravitational
wave background (SGWB) at frequencies detectable by the LISA detector. We develop tools …

Future missions of gravitational-wave astronomy will be operated by space-based
interferometers, covering a very wide range of frequencies. Search for stochastic …

The space-based gravitational wave detector LISA will observe mergers of massive black
hole binary systems (MBHBs) to cosmological distances, as well as inspiralling stellar-origin …

Numerical relativists can now produce gravitational waveforms with memory effects routinely
and accurately. The gravitational-wave memory effect contains very low-frequency …

Abstract Space-borne interferometric gravitational wave detectors, sensitive in the low-
frequency (millihertz) band, will fly in the next decade. In these detectors the spacecraft-to …