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The status of LCGT

Kazuaki Kuroda and the LCGT Collaboration

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The current status of LCGT is described. The physical target of LCGT is to detect every year at least one event of gravitational wave signal produced at the coalescence of a binary neutron star. To attain this objective, LCGT is built underground by adopting cryogenic mirrors with a high power laser. To assure the reliable detection, two independent sets of interferometers are installed in a common vacuum system.


PACS

04.80.Nn Gravitational wave detectors and experiments

95.55.Ym Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques

07.20.Mc Cryogenics; refrigerators, low-temperature equipment

07.60.Ly Interferometers

97.60.Jd Neutron stars

MSC

78A60 Lasers, masers, optical bistability, nonlinear optics (See also 81V80)

83C35 Gravitational waves

85A05 Galactic and stellar dynamics

Subjects

Instrumentation and measurement

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 8 (21 April 2006)

Received 10 October 2005, in final form 23 December 2006

Published 28 March 2006



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