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KAGRA (Large Cryogenic Gravitational Wave Telescope) Project is jointly promoted by Institute for Cosmic Ray Research (ICRR, the main host), National Astronomical Observatory of Japan (NAOJ), High Energy Accelerator Research Organization (KEK) and other member institutes as an international collaboration.

March 31, 2014
Excavation of the KAGRA tunnel has been completed.
At the end of March 2014, the excavation of the KAGRA tunnels, which span more than 7 km, has been successfully completed.

KAGRA Project (presented by ICRR)
Accelerating masses generate gravitational waves which are distortions in the structure of spacetime and propagate like ripples through the Universe. Although they were theoretically predicted from Einstein's General Theory of Relativity about 100 years ago, there has not yet been a direct detection of gravitational waves, mainly because their interaction with matter is extremely weak. The first indirect evidence for the existence of gravitational waves came from the discovery and subsequent observations of a binary pulsar system by Hulse and Taylor, for which they received Nobel prizes in 1993.
A recent report from the BICEP2 project about the observation of a B-mode polarization component in the cosmic microwave background will, if confirmed, add more support for the existence of gravitational waves. With the indirect evidence piling up, the importance of directly detecting gravitational wave has never been higher.

Until now, most astronomical observations have used electromagnetic waves to extract information from sources. Since the generation mechanism for gravitational waves is vastly different from the generation mechanism for electromagnetic waves, gravitational waves carry unique information about the sources which is otherwise unavailable to us. Direct detection of gravitational waves from astronomical sources will give us rich opportunities to explore the physics of extreme conditions, such as the equation of state of neutron stars, the direct measurement of black hole parameters, and the explosion mechanism of supernovae.

KAGRA is an L-shaped laser interferometric gravitational wave detector with a 3 km baseline length being built in the underground site of Kamioka mine in Gifu prefecture, Japan. Using this interferometer, we try to detect tiny distortion of spacetime as small as one 10 billionth of the diameter of a hydrogen atom. In order to achieve such an extreme sensitivity, external disturbances such as ground vibrations have to be eliminated. The ground vibrations of the Kamioka-mine are about 100 times smaller than those of Tokyo. This seismically quiet environment is essential for the success of KAGRA. This is why we excavated long tunnels with a total length of 7,697 m.

inside the tunnel (presented by ICRR)
Once operational, KAGRA is expected to open a completely new observational window to the Universe.

The National Astronomical Observatory of Japan (NAOJ) is one of the core institutes of the KAGRA project, together with the Institute for Cosmic Ray Research, University of Tokyo and the High Energy Accelerator Research Organization, promoting the construction and operation of KAGRA. The completion of the tunnel excavation marks an important milestone for the construction of KAGRA. For more details, please refer to the press release from the University of Tokyo.

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contact: gw-webmaster@  Add following strings : nao.ac.jp
Last updated 31/03/2014