文献

J-GLOBAL ID：202002283946172591   整理番号：20A2535076

中性子星極端物質観測所:グローバルネットワークにおけるキロヘルツバンド重力波検出器【JST・京大機械翻訳】

Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network

著者 (119件)： Ackley K. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Adya V. B. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Agrawal P. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Altin P. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Ashton G. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Bailes M. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Baltinas E. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Barbuio A. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Beniwal D. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Blair C. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Blair D. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Bolingbroke G. N. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Bossilkov V. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Shachar Boublil S. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Brown D. D. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Burridge B. J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Calderon Bustillo J. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Calderon Bustillo J. (The Chinese University of Hong Kong, Shatin, NT, Hong Kong) ,  Cameron J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Tuong Cao H. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Carlin J. B. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Chang S. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Charlton P. (Charles Sturt University, Wagga Wagga, NSW 2678, Australia) ,  Chatterjee C. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Chattopadhyay D. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Chen X. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Chi J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Chow J. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Chu Q. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Ciobanu A. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Clarke T. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Clearwater P. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Clearwater P. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Cooke J. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Coward D. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Crisp H. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Dattatri R. J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Deller A. T. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Dobie D. A. (Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006, Australia) ,  Dobie D. A. (ATNF, CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710, Australia) ,  Dunn L. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Easter P. J. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Eichholz J. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Evans R. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Flynn C. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Foran G. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Forsyth P. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Gai Y. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Galaudage S. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Galloway D. K. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Gendre B. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Goncharov B. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Goode S. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Gozzard D. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Grace B. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Graham A. W. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Heger A. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Hernandez Vivanco F. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Hirai R. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Holland N. A. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Holmes Z. J. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Howard E. (Department of Physics and Astronomy, Macquarie University, Sydney, NSW 2109, Australia) ,  Howard E. (Centre for Quantum Dynamics, Griffith University, Brisbane, Australia) ,  Howell E. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Howitt G. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Huebner M. T. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Hurley J. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Ingram C. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Jaberian Hamedan V. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Jenner K. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Ju L. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Kapasi D. P. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Kaur T. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Kijbunchoo N. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Kovalam M. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Kumar Choudhary R. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Lasky P. D. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Lau M. Y. M. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Leung J. (Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006, Australia) ,  Liu J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Loh K. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Mailvagan A. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Mandel I. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  McCann J. J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  McClelland D. E. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  McKenzie K. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  McManus D. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  McRae T. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Melatos A. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Meyers P. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Middleton H. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Miles M. T. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Millhouse M. (OzGrav, School of Physics, University of Melbourne, Parkville, VIC 3010, Australia) ,  Lun Mong Y. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Mueller B. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Munch J. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Musiov J. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Muusse S. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Nathan R. S. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Naveh Y. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Neijssel C. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Neijssel C. (University of Birmingham, Birmingham, B15 2TT, UK) ,  Neil B. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Ng S. W. S. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Oloworaran V. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Ottaway D. J. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Page M. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Pan J. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Pathak M. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Payne E. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Powell J. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Pritchard J. (Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006, Australia) ,  Puckridge E. (OzGrav, University of Adelaide, Adelaide, SA 5005, Australia) ,  Raidani A. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Rallabhandi V. (OzGrav, University of Western Australia, Crawley, WA 6009, Australia) ,  Reardon D. (OzGrav, Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia) ,  Riley J. A. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia) ,  Roberts L. (OzGrav, ANU Centre for Gravitational Astrophysics, Research Schools of Physics, and Astronomy and Astrophysics, The Australian National University, Canberra, ACT 2601, Australia) ,  Romero-Shaw I. M. (OzGrav, School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia)
資料名： Publications of the Astronomical Society of Australia  (Publications of the Astronomical Society of Australia)
巻： 37  ページ： e047  発行年： 2020年 
JST資料番号： W5500A  ISSN： 1323-3580  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： イギリス (GBR)  言語： 英語 (EN)

抄録/ポイント： 合体中性子星からの重力波は,極端な密度で核物質に関する情報を符号化し,実験室実験によってアクセスできない。遅い吸入は潮汐の存在に影響され,それは中性子星状態方程式に依存する。中性子星合併は重力波を放射する急速に回転する残留中性子星を生成することが期待されている。これらは,非常にホットなポストマーガー環境に対する手がかりを提供するであろう。重力波における核物質のこの特徴は,現在の検出器の最も敏感なバンドの外側である2~4kHz周波数帯におけるほとんどの情報を含む。中性子星極端散乱(NEMO)のための設計概念と科学事例を示し,中性子星を併合する核物理学を研究するために最適化した重力波干渉計を最適化した。この概念は,高循環レーザパワー,量子スクイージング,および重力波を用いた核物質プローブに必要な高周波感度を達成するために特別に設計された検出器トポロジーを使用する。1kHz以上では,提案した歪感度は,コストの一部で完全第三世代検出器に匹敵する。このような感度変化は,2つのA+検出器が数年あたり約1年間,約1年あたり約1年間から数年間まで,また,超新星,孤立中性子星,および他のエキゾチックの重力波観測を可能にする,事象速度を予想する。Please refer to the publisher for the copyright holders. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 位相幾何学 ,  核物質 ,  干渉計 ,  最適化 ,  散乱 ,  状態方程式 ,  *中性子 ,  *中性子星 ,  超新星 ,  潮汐 ,  HF【周波数】 ,  レーザ出力 ,  スクイージング ,  周波数帯
準シソーラス用語： *重力波検出器 , 【Automatic Indexing@JST】

著者キーワード (4件)： 状態方程式 ,  重力波星:中性子 ,  計装:検出器 ,  計装:干渉計

分類 (2件)： 恒星  (DB05000P) ,  重力理論の実験的試験及び観測  (BA07040Q)

タイトルに関連する用語 (5件)： 中性子星 ,  物質 ,  観測所 ,  グローバル ,  重力波検出器