論文 ·日本語 ·未確認
Detector configuration of KAGRA–the Japanese cryogenic gravitational-wave detector
- 刊行年
- 2012-06-01
- 収録
- 『Classical and Quantum Gravity』 29(12) pp. 124007-124007
- 出版
- IOP Publishing
- 言語
- 英語
- OpenAlex
- W2119896891
- DOI
- 10.1088/0264-9381/29/12/124007
- MAG
- 2119896891
- ISSN
- 0264-9381
- URL
- https://iopscience.iop.org/article/10.1088/0264-9381/29/12/124007/pdf
要旨
Abstract The construction of the Japanese second-generation gravitational-wave detector KAGRA (previously called LCGT) has been started. In the next 6–7 years, we will be able to observe the spacetime ripple from faraway galaxies. KAGRA is equipped with the latest advanced technologies. The entire 3 km long detector is located in the underground to be isolated from the seismic motion, the core optics are cooled down to 20 K to reduce thermal fluctuations and quantum non-demolition techniques are used to decrease quantum noise. In this paper, we introduce the detector configuration of KAGRA, its design, strategy and downselection of parameters.
主題
この書誌の出所
- openalex— W2119896891（2026-08-14取得）
引用
Kentaro Somiya（2012-06-01） Detector configuration of KAGRA–the Japanese cryogenic gravitational-wave detector 『Classical and Quantum Gravity』 29(12) pp. 124007-124007 IOP Publishing