Current Status of TAMA300

Details Current Status of TAMA300 Current Status of TAMA300

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.3093s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

A Japanese laser interferometer gravitational wave antenna, TAMA300, has been developed and recently a power recycling system was implemented. The interferometer is finally operating in the designed optical configuration, with improved sensitivity, 1 × 10-18 mHz-1/2 in displacement at around 1 kHz. With this sensitivity the antenna can be expected to have an ability to sense the spacetime strain caused by the coalescence of neutron star binaries within our galaxy with a signal to noise ratio better than 40. In this paper, the implementation of the recycling system and the corresponding improvement in the sensitivity are reported in addition to the review of the system.

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