Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 23, Issue 8, Pages S215-S221Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/23/8/S27
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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.
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