Towards Detection of Gravitational Waves

Details Towards Detection of Gravitational Waves Towards Detection of Gravitational Waves

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005grg..conf...24b&link_type=abstract

GENERAL RELATIVITY AND GRAVITATION. Proceedings of the 17th International Conference. Held 18-23 July 2004 in RDS Convention Cen

Computer Science

1

Scientific paper

The status, progress and plans for the Interferometer Gravitational Wave Detectors are presented. Resonant Bar and Interferometric detectors are complementary approaches to gravitational wave detection. Resonant Bars are generally narrow band cryogenic detectors sensitive at frequencies of about 1 KHz. Interferometers are long baseline broad-band detectors covering a frequencies range of about 10 to 104 Hz, having sensitivity to lower frequency gravitational radiation. In this presentation I review the techniques and status of both the resonant bar detectors and gravitational wave interferometers worldwide.

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