التفاصيل البيبلوغرافية
العنوان:
Radiative Cooling of the Thermally Isolated System in KAGRA Gravitational Wave Telescope
المؤلفون:
A. Hagiwara , C-Y. Lin , Akito Araya , T. Kajita , M. A. Barton , R. Bajpai , Yoshiaki Himemoto , I. M. Pinto , G. Kang , M. H. P. M. van Putten , K. Miyo , K. Oohara , Tatsuhiro Yamada , Satoshi Tsuchida , Yoshiyuki Obuchi , T. Shimoda , P. Jung , M. Fukunaga , G-Z. Huang , Yuichiro Sekiguchi , B. H. Hsieh , Yuki Inoue , S. Shibagaki , Albert K. H. Kong , K. Chen , Yoshihiko Saito , H. C. Wu , Shigeo Nagano , Kei Kotake , Hisa-aki Shinkai , S. Wu , T. Shishido , R. Nakashima , T. Yoshioka , R. Flaminio , Hiroyuki Takeda , T. Narikawa , Keiko Kokeyama , S. Oshino , Takashi Uchiyama , John J. Oh , H. W. Lee , Soichiro Morisaki , G. Ge , S. Sato , Nobuyuki Kanda , N. Hirata , Y. Tomigami , A. Ueda , Yasufumi Kojima , Kunihito Ioka , Hajime Sotani , Chunglee Kim , Nobutada Kimura , H. K. Tanaka , Sakae Araki , Takahiro Tanaka , Yi Chen , Eiichi Hirose , Kouji Nakamura , F. Travasso , Hirotaka Takahashi , Kipp Cannon , T. Kawasaki , Osamu Miyakawa , D. Tuyenbayev , Fumihiro Uraguchi , Shinji Miyoki , Y. Sakuno , L. W. Luo , F-L. Lin , Wei-Tou Ni , H. Vocca , Masatake Ohashi , Toshio Suzuki , Jong-Dae Park , Takashi Sato , H. Pang , Mitsuhiro Fukushima , Koki Okutomi , K. Yamamoto , Ray-Kuang Lee , Sadakazu Haino , M. Nakano , F. E. Peiia Arellano , Kimio Tsubono , Hyun Lee , S. Imam , Naoko Ohishi , Yuka Fujii , Jinsook Kim , Sachiko Kuroyanagi , Y. Bae , G. Ueshima , Toshihiro Tsuzuki , Y. K. Chu , T. Tomura , Kohei Inayoshi , M. Marchio , S. Tanioka , Kyohei Kawaguchi , Souichi Telada , T. Sawada , T. Yokozawa , J. Z. Wang , K. Yokogawa , Yuta Michimura , B. Ikenoue , T. Sekiguchi , H. Yuzurihara , K. Hasegawa , Jun'ichi Yokoyama , E. N. Tapia San Martin , M. Leonardi , K. Jung , C. M. Kuo , W. S. Kim , Tomotada Akutsu , H-S. Kuo , N. Kawai , Zong-Hong Zhu , R. Sugimoto , Rajesh Kumar , Haruki Kitazawa , R. Kozu , Shuji Saito , K. Izumi , T. Yamamoto , K. Kusayanagi , Y. M. Kim , E. Capocasa , Kyujin Kwak , Seog Oh , Hideaki Hayakawa , Koji Arai , H. Chu , Y. Miyazaki , L. Trozzo , Norichika Sago , Atsushi Nishizawa , Koh Ueno , Y. Moriwaki , Guo-Chin Liu , S. Bae , C. M. Wu , Y. Hiranuma , W-R. Xu , C. P. Ooi , Kazuhiro Hayama , Y. Sakai , K. Sakai , R. Shimizu , L. C.-C. Lin , M. Chan , Kentaro Somiya , Edwin J. Son , Yoshio Arai , Masaki Ando , C. Chen , Naoki Aritomi , Ryutaro Takahashi , Akiteru Takamori , Chihiro Kozakai , Takayuki Tomaru , M. Takeda , K. Shimode , Yuhang Zhao , Hiroyuki Nakano , Yutaro Enomoto , W. Ogaki , Z. Hong , Masashi Ohkawa , Y. Aso , P. W. Huang , Y. Huang , Kazuyuki Tanaka , S. Takano , J. Kume , Norikatsu Mio , T. Uehara , Kentaro Komori , Hideyuki Tagoshi , N. Kita , T. Tsang , N. Uchikata , Kuo-Chuan Pan , R. Negishi , S. Eguchi , A. Shoda , T. Ushiba , Simon Zeidler , Luca Baiotti , Yousuke Itoh , Koji Nagano , M. Kamiizumi , A. Miyamoto
المساهمون:
Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), KAGRA
المصدر:
J.Phys.Conf.Ser.
بيانات النشر:
HAL CCSD, 2020.
سنة النشر:
2020
مصطلحات موضوعية:
History , Radiative cooling , Thermally isolated system , detector: noise , cavity: optical , 01 natural sciences , Education , law.invention , Telescope , fluctuation: thermal , law , 0103 physical sciences , noise: thermal , KAGRA , laser: interferometer , [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] , 010306 general physics , mirror , Physics , radiation: thermal , 010308 nuclear & particles physics , Gravitational wave , gravitational radiation , Astronomy , gravitational radiation detector , Computer Science Applications , injection , cryogenics , specific heat
الوصف:
Radiative cooling of the thermally isolated system is investigated in KAGRA gravitational wave telescope. KAGRA is a laser interferometer-based detector and main mirrors constituting optical cavities are cool down to 20K to reduce noises caused by the thermal fluctuation. The mirror is suspended with the multi-stage pendulum to isolate any vibration. Therefore, this mirror suspension system has few heat links to reduce vibration injection. Thus, this system is mainly cooled down with thermal radiation. In order to understand the process of radiative cooling of the mirror, we analyzed cooling curve based on mass and specific heat. As a result, it was newly found that a cryogenic part called ”cryogenic duct-shield” seems to have large contribution in the beginning of the mirror cooling. This finding will help to design new cooling system for the next generation cryogenic gravitational wave detector.
وصف الملف:
application/pdf
اللغة:
English
تدمد:
1742-6588
DOI:
10.1088/1742-6596/1857/1/012002⟩
URL الوصول:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ba446ae87fea2e74ba9fef64ef23efc https://hal.archives-ouvertes.fr/hal-03210395
Rights:
OPEN
رقم الانضمام:
edsair.doi.dedup.....2ba446ae87fea2e74ba9fef64ef23efc
قاعدة البيانات:
OpenAIRE