Overview Of Kagra: Detector Design And Construction History

Akutsu T.,Ando M.,Arai K., Arai Y.,Araki S.,Araya A.,Aritomi N.,Aso Y., Bae S. -W.,Bae Y. -B.,Baiotti L.,Bajpai R.,Barton M. A.,Cannon K., Capocasa E.,Chan M. -L.,Chen C. -S.,Chen K. -H., Chen Y. -R.,Chu H. -Y.,Chu Y-K.,Eguchi S.,Enomoto Y.,Flaminio R.,Fujii Y.,Fukunaga M., Fukushima M.,Ge G. -G.,Hagiwara A.,Haino S., Hasegawa K., Hayakawa H.,Hayama K.,Himemoto Y.,Hiranuma Y.,Hirata N., Hirose E.,Hong Z.,Hsieh B. -H., Huang G. -Z.,Huang P. -W.,Huang Y. -J.,Ikenoue B.,Imam S.,Inayoshi K., Inoue Y.,Ioka K.,Itoh Y.,Izumi K., Jung K.,Jung P.,Kajita T.,Kamiizumi M.,Kanda N., Kang G. -W.,Kawaguchi K., Kawai N.,Kawasaki T.,Kim C.,Kim J., Kim W.,Kim Y. -M.,Kimura N.,Kita N.,Kitazawa H., Kojima Y.,Kokeyama K.,Komori K.,Kong A. K. H.,Kotake K.,Kozakai C.,Kozu R.,Kumar R.,Kume J., Kuo C. -M.,Kuo H. -S.,Kuroyanagi S.,Kusayanagi K.,Kwak K.,Lee H. -K., Lee H. -W.,Lee R. -K.,Leonardi M., Lin C. -Y.,Lin F. -L.,Lin L. C. -C.,Liu G. -C.,Luo L. -W.,Marchio M.,Michimura Y.,Mio N.,Miyakawa O.,Miyamoto A., Miyazaki Y.,Miyo K.,Miyoki S.,Morisaki S.,Moriwaki Y., Nagano K.,Nagano S.,Nakamura K.,Nakano H.,Nakano M.,Nakashima R.,Narikawa T.,Negishi R.,Ni W. -T.,Nishizawa A.,Obuchi Y.,Ogaki W.,Oh J. J., Oh S. -H., Ohashi M.,Ohishi N.,Ohkawa M.,Okutomi K.,Oohara K.,Ooi C. -P.,Oshino S.,Pan K. -C., Pang H. -F.,Park J.,Arellano F. E. Peña,Pinto I.,Sago N.,Saito S.,Saito Y., Sakai K., Sakai Y.,Sakuno Y., Sato S., Sato T., Sawada T., Sekiguchi T.,Sekiguchi Y.,Shibagaki S.,Shimizu R.,Shimoda T.,Shimode K.,Shinkai H.,Shishido T.,Shoda A., Somiya K.,Son E. J.,Sotani H.,Sugimoto R.,Suzuki T.,Tagoshi H.,Takahashi H.,Takahashi R.,Takamori A., Takano S.,Takeda H.,Takeda M.,Tanaka H.,Tanaka K., Tanaka T.,Tanioka S.,Martin E. N. Tapia San,Telada S.,Tomaru T.,Tomigami Y., Tomura T.,Travasso F.,Trozzo L.,Tsang T. T. L.,Tsubono K.,Tsuchida S.,Tsuzuki T., Tuyenbayev D.,Uchikata N., Uchiyama T.,Ueda A., Uehara T.,Ueno K.,Ueshima G.,Uraguchi F.,Ushiba T.,van Putten M. H. P. M.,Vocca H.,Wang J., Wu C. -M., Wu H. -C.,Wu S. -R., Xu W. -R.,Yamada T.,Yamamoto Ka.,Yamamoto Ko.,Yamamoto T.,Yokogawa K.,Yokoyama J.,Yokozawa T.,Yoshioka T.,Yuzurihara H.,Zeidler S.,Zhao Y.,Zhu Z. -H.

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS（2021）

引用 167|浏览138

暂无评分

摘要

KAGRA is a newly built gravitational-wave telescope, a laser interferometer comprising arms with a length of 3 km, located in Kamioka, Gifu, Japan. KAGRA was constructed under the ground and it is operated using cryogenic mirrors that help in reducing the seismic and thermal noise. Both technologies are expected to provide directions for the future of gravitational-wave telescopes. In 2019, KAGRA finished all installations with the designed configuration, which we call the baseline KAGRA. For this occasion, we present an overview of the baseline KAGRA from various viewpoints in a series of articles. In this article, we introduce the design configurations of KAGRA with its historical background.

查看译文

关键词

detector design,kagra,construction

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要