TAMA project: Design and current status

Details TAMA project: Design and current status TAMA project: Design and current status

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..523..128a&link_type=abstract

GRAVITATIONAL WAVES: Third Edoardo Amaldi Conference. AIP Conference Proceedings, Volume 523, pp. 128-139 (2000).

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Gravitational Wave Detectors And Experiments, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

TAMA is a Japanese project to construct and operate an interferometric gravitational-wave detector with a baseline length of 300 m at the Mitaka campus of National Astronomical Observatory in Tokyo. The aim of this project is to develop techniques necessary for future large-scale interferometers and, moreover, to detect gravitational waves generated within our local group of galaxies. Now, stable operation of the TAMA300 interferometer has been realized under the final configuration, except for power recycling with a displacement noise level of 6×10-18 m/Hz. The interferometer was operated continuously over 7 hours without unlock. In this article, the design of the TAMA300 interferometer is reviewed, and its current status of development is reported. .

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