Expected sources and data analysis on laser interferometric gravitational wave detector

Details Expected sources and data analysis on laser interferometric gravitational wave detector Expected sources and data analysis on laser interferometric gravitational wave detector

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001asthe..94..448k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 94, No. 10, p. 448 - 456 (2001)

Physics

Gravitational Wave Detectors

Scientific paper

The direct detection of gravitational wave has been expected for physics in strong gravitational field, and for a new deep probe for astronomical objects. Recently, some projects of large-scale laser interferometric gravitational wave detector compete for the first detection of gravitational wave. Our project TAMA300 which is placed in NAOJ, achieved worlds best sensitivity and long stable operation as a realistic observatory. In this document, we will give a brief description of gravitational wave detection, expected sources, and TAMA's data analysis.

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