Any slight variations in the fundamental constants of nature, which may be induced by dark
matter or some yet-to-be-discovered cosmic field, would characteristically alter the phase of …

We performed a detailed analysis of the detectability of a wide range of gravitational waves
derived from core-collapse supernova simulations using gravitational-wave detector noise …

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

Coincident observations with gravitational wave (GW) detectors and other astronomical
instruments are among the main objectives of the experiments with the network of LIGO …

The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in
early 2005, collected data with significantly lower noise than previous science runs. We …

Presented in this paper is a technique that we propose for extracting the physical
parameters of a rotating stellar core collapse from the observation of the associated …

We report on the first joint search for gravitational waves by the TAMA and LIGO
collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in …

The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a
new collaborative effort between the numerical relativity community and the data analysis …

TAMA300, an interferometric gravitational-wave detector with a 300 m baseline length, has
been developed and operated with sufficient sensitivity to detect gravitational-wave events …

This thesis explores the possibility of searching for new effects of dark matter that are linear
in g, an approach that offers enormous advantages over conventional schemes, since the …