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J-GLOBAL ID：201902234288125274   整理番号：19A0548928

GW170817:コンパクト連星合体からの確率的重力波背景に対する意味【JST・京大機械翻訳】

GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

著者 (120件)： Abbott B. P. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Abbott R. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Abbott T. D. (Louisiana State University, Baton Rouge, Louisiana 70803, USA) ,  Acernese F. (Universita di Salerno, Fisciano, I-84084 Salerno, Italy) ,  Acernese F. (INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy) ,  Ackley K. (University of Florida, Gainesville, Florida 32611, USA) ,  Ackley K. (OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia) ,  Adams C. (LIGO Livingston Observatory, Livingston, Louisiana 70754, USA) ,  Adams T. (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), Universite Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France) ,  Addesso P. (University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy) ,  Adhikari R. X. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Adya V. B. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Affeldt C. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Afrough M. (The University of Mississippi, University, Mississippi 38677, USA) ,  Agarwal B. (NCSA, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA) ,  Agathos M. (University of Cambridge, Cambridge CB2 1TN, United Kingdom) ,  Agatsuma K. (Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands) ,  Aggarwal N. (LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA) ,  Aguiar O. D. (Instituto Nacional de Pesquisas Espaciais, 12227-010 Sao Jose dos Campos, Sao Paulo, Brazil) ,  Aiello L. (Gran Sasso Science Institute (GSSI), I-67100 L’Aquila, Italy) ,  Aiello L. (INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy) ,  Ain A. (Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India) ,  Ajith P. (International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India) ,  Allen B. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Allen B. (University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA) ,  Allen B. (Leibniz Universitaet Hannover, D-30167 Hannover, Germany) ,  Allen G. (NCSA, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA) ,  Allocca A. (Universita di Pisa, I-56127 Pisa, Italy) ,  Allocca A. (INFN, Sezione di Pisa, I-56127 Pisa, Italy) ,  Altin P. A. (OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia) ,  Amato A. (Laboratoire des Materiaux Avances (LMA), CNRS/IN2P3, F-69622 Villeurbanne, France) ,  Ananyeva A. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Anderson S. B. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Anderson W. G. (University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA) ,  Angelova S. V. (SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom) ,  Antier S. (LAL, Univ. Paris-Sud, CNRS/IN2P3, Universite Paris-Saclay, F-91898 Orsay, France) ,  Appert S. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Arai K. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Araya M. C. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Areeda J. S. (California State University Fullerton, Fullerton, California 92831, USA) ,  Arnaud N. (LAL, Univ. Paris-Sud, CNRS/IN2P3, Universite Paris-Saclay, F-91898 Orsay, France) ,  Arnaud N. (European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy) ,  Arun K. G. (Chennai Mathematical Institute, Chennai 603103, India) ,  Ascenzi S. (Universita di Roma Tor Vergata, I-00133 Roma, Italy) ,  Ascenzi S. (INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy) ,  Ashton G. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Ast M. (Universitaet Hamburg, D-22761 Hamburg, Germany) ,  Aston S. M. (LIGO Livingston Observatory, Livingston, Louisiana 70754, USA) ,  Astone P. (INFN, Sezione di Roma, I-00185 Roma, Italy) ,  Atallah D. V. (Cardiff University, Cardiff CF24 3AA, United Kingdom) ,  Aufmuth P. (Leibniz Universitaet Hannover, D-30167 Hannover, Germany) ,  Aulbert C. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  AultONeal K. (Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA) ,  Austin C. (Louisiana State University, Baton Rouge, Louisiana 70803, USA) ,  Avila-Alvarez A. (California State University Fullerton, Fullerton, California 92831, USA) ,  Babak S. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam-Golm, Germany) ,  Bacon P. (APC, AstroParticule et Cosmologie, Universite Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cite, F-75205 Paris Cedex 13, France) ,  Bader M. K. M. (Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands) ,  Bae S. (Korea Institute of Science and Technology Information, Daejeon 34141, Korea) ,  Baker P. T. (West Virginia University, Morgantown, West Virginia 26506, USA) ,  Baldaccini F. (Universita di Perugia, I-06123 Perugia, Italy) ,  Baldaccini F. (INFN, Sezione di Perugia, I-06123 Perugia, Italy) ,  Ballardin G. (European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy) ,  Ballmer S. W. (Syracuse University, Syracuse, New York 13244, USA) ,  Banagiri S. (University of Minnesota, Minneapolis, Minnesota 55455, USA) ,  Barayoga J. C. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Barclay S. E. (SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom) ,  Barish B. C. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Barker D. (LIGO Hanford Observatory, Richland, Washington 99352, USA) ,  Barkett K. (Caltech CaRT, Pasadena, California 91125, USA) ,  Barone F. (Universita di Salerno, Fisciano, I-84084 Salerno, Italy) ,  Barone F. (INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy) ,  Barr B. (SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom) ,  Barsotti L. (LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA) ,  Barsuglia M. (APC, AstroParticule et Cosmologie, Universite Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cite, F-75205 Paris Cedex 13, France) ,  Barta D. (Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklos ut 29-33, Hungary) ,  Bartlett J. (LIGO Hanford Observatory, Richland, Washington 99352, USA) ,  Bartos I. (Columbia University, New York, New York 10027, USA) ,  Bartos I. (University of Florida, Gainesville, Florida 32611, USA) ,  Bassiri R. (Stanford University, Stanford, California 94305, USA) ,  Basti A. (Universita di Pisa, I-56127 Pisa, Italy) ,  Basti A. (INFN, Sezione di Pisa, I-56127 Pisa, Italy) ,  Batch J. C. (LIGO Hanford Observatory, Richland, Washington 99352, USA) ,  Bawaj M. (Universita di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy) ,  Bawaj M. (INFN, Sezione di Perugia, I-06123 Perugia, Italy) ,  Bayley J. C. (SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom) ,  Bazzan M. (Universita di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy) ,  Bazzan M. (INFN, Sezione di Padova, I-35131 Padova, Italy) ,  Becsy B. (Institute of Physics, Eotvos University, Pazmany P. s. 1/A, Budapest 1117, Hungary) ,  Beer C. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Bejger M. (Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716 Warsaw, Poland) ,  Belahcene I. (LAL, Univ. Paris-Sud, CNRS/IN2P3, Universite Paris-Saclay, F-91898 Orsay, France) ,  Bell A. S. (SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom) ,  Berger B. K. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Bergmann G. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Bero J. J. (Rochester Institute of Technology, Rochester, New York 14623, USA) ,  Berry C. P. L. (University of Birmingham, Birmingham B15 2TT, United Kingdom) ,  Bersanetti D. (INFN, Sezione di Genova, I-16146 Genova, Italy) ,  Bertolini A. (Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands) ,  Betzwieser J. (LIGO Livingston Observatory, Livingston, Louisiana 70754, USA) ,  Bhagwat S. (Syracuse University, Syracuse, New York 13244, USA) ,  Bhandare R. (RRCAT, Indore, Madhya Pradesh 452013, India) ,  Bilenko I. A. ,  Billingsley G. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Billman C. R. (University of Florida, Gainesville, Florida 32611, USA) ,  Birch J. (LIGO Livingston Observatory, Livingston, Louisiana 70754, USA) ,  Birney R. ,  Birnholtz O. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany) ,  Biscans S. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Biscans S. (LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA) ,  Biscoveanu S. ,  Biscoveanu S. (OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia) ,  Bisht A. (Leibniz Universitaet Hannover, D-30167 Hannover, Germany) ,  Bitossi M. (European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy) ,  Bitossi M. (INFN, Sezione di Pisa, I-56127 Pisa, Italy) ,  Biwer C. (Syracuse University, Syracuse, New York 13244, USA) ,  Bizouard M. A. (LAL, Univ. Paris-Sud, CNRS/IN2P3, Universite Paris-Saclay, F-91898 Orsay, France) ,  Blackburn J. K. (LIGO, California Institute of Technology, Pasadena, California 91125, USA) ,  Blackman J. (Caltech CaRT, Pasadena, California 91125, USA) ,  Blair C. D. (LIGO, California Institute of Technology, Pasadena, California 91125, USA)
資料名： Physical Review Letters  (Physical Review Letters)
巻： 120  号： 9  ページ： 091101  発行年： 2018年 
JST資料番号： H0070A  ISSN： 0031-9007  CODEN： PRLTAO  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： アメリカ合衆国 (USA)  言語： 英語 (EN)

抄録/ポイント： LIGO科学とVirgo共同研究は,2つの中性子星の合体からの重力波の最初の検出であるイベントGW170817を発表した。このイベントから推定された二元中性子星の合併率は,遠い非分解性二元中性子星が,顕著な天体物理的確率的重力波背景を生成することを示唆する。二元中性子星成分は二成分ブラックホールからの寄与に付加し,これまでの予想に対して全天体物理的背景の振幅を増加させる。先進的なLIGO-Virgo周波数帯において,確率的背景(約25Hz)に最も敏感な,2元ブラックホールのみからの[数式:原文を参照]と比較して,90%の信頼度で振幅[数式:原文を参照]を有する全天体物理的背景を予測した。コンパクトな二値合併症に対する最も可能性のある速度を仮定して,全観測時間の40か月後に,全バックグラウンドが検出可能であることを見出した。これは,Advanced LIGOとVirgoに対する期待されるタイミングに基づいて,それらの設計感度に到達する。Copyright 2019 The American Physical Society All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 中性子星 ,  合併症 ,  周波数帯 ,  信頼度 ,  宇宙物理学 ,  *連星 ,  ブラックホール
準シソーラス用語： LIGO , 【Automatic Indexing@JST】

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 (6件)： GW170817 ,  コンパクト ,  連星合体 ,  確率 ,  重力波背景 ,  意味