In this perspective, we outline that a space borne gravitational wave detector network
combining LISA and Taiji can be used to measure the Hubble constant with an uncertainty …

The first generation of long-baseline laser interferometric detectors of gravitational waves
will start collecting data in 2001–2003. We carefully analyse their planned performance and …

The space gravitational wave (GW) antennae is more sensitive to the lower frequency GW
signals compare with the ground-based GW detectors. The space mission Taiji is designed …

It has recently been suggested that the presence of a plenitude of light axions, an Axiverse,
is evidence for the extra dimensions of string theory. We discuss the observational …

We propose a cosmological scenario in which the hot big bang universe is produced by the
collision of a brane in the bulk space with a bounding orbifold plane, beginning from an …

It may be possible to construct a laser interferometer gravitational wave antenna in space
with h rms∼ 10− 27 at f∼ 0.1 Hz in this century. Using this antenna,(1) typically 10 5 chirp …

The Advanced Laser Interferometer Antenna (ALIA) and the Big Bang Observer (BBO) have
been proposed as follow on missions to the Laser Interferometer Space Antenna (LISA) …

Laser frequency noise is a dominant noise background for the detection of gravitational
waves using long-baseline optical interferometry. Amelioration of this noise requires near …

Massive black hole binary systems, with masses in the range∼ 104–1010M⊙, are among
the primary sources of gravitational waves in the frequency window∼ 10− 9–0.1 Hz. Pulsar …

Double white dwarfs (DWDs) will be the most numerous gravitational-wave (GW) sources for
the Laser Interferometer Space Antenna (LISA). Most of the Galactic DWDs will be …