Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

被引：818

作者：

Abbott, B. P. ^{[1
]}

Abbott, R. ^{[1
]}

Abbott, T. D. ^{[2
]}

Abernathy, M. R. ^{[3
]}

Acernese, F. ^{[4
,5
]}

Ackley, K. ^{[6
]}

Adams, C. ^{[7
]}

Adams, T. ^{[8
]}

Addesso, P. ^{[9
,10
]}

Adhikari, R. X. ^{[1
]}

Adya, V. B. ^{[11
]}

Affeldt, C. ^{[11
]}

Agathos, M. ^{[12
]}

Agatsuma, K. ^{[12
]}

Aggarwal, N. ^{[13
]}

Aguiar, O. D. ^{[14
]}

Aiello, L. ^{[15
,16
]}

Ain, A. ^{[1
,17
]}

Ajith, P. ^{[18
]}

Akutsu, T. ^{[19
]}

Allen, B. ^{[11
,20
,21
]}

Allocca, A. ^{[22
,23
]}

Altin, P. A. ^{[24
]}

Ananyeva, A. ^{[1
]}

Anderson, S. B. ^{[1
]}

Anderson, W. G. ^{[20
]}

Ando, M. ^{[19
,25
,26
]}

Appert, S. ^{[1
]}

Arai, K. ^{[1
]}

Araya, A. ^{[27
]}

Araya, M. C. ^{[1
]}

Areeda, J. S. ^{[28
]}

Arnaud, N. ^{[29
]}

Arun, K. G. ^{[30
]}

Asada, H. ^{[31
]}

Ascenzi, S. ^{[16
,32
]}

Ashton, G. ^{[11
]}

Aso, Y. ^{[19
]}

Ast, M. ^{[33
]}

Aston, S. M. ^{[7
]}

Astone, P. ^{[34
]}

Atsuta, S. ^{[35
]}

Aufmuth, P. ^{[21
]}

Aulbert, C. ^{[11
]}

Avila-Alvarez, A. ^{[28
]}

Awai, K. ^{[36
]}

Babak, S. ^{[37
]}

Bacon, P. ^{[38
]}

Bader, M. K. M. ^{[12
]}

Baiotti, L. ^{[39
]}

机构：

[1] CALTECH, LIGO, Pasadena, CA 91125 USA

[2] Louisiana State Univ, Baton Rouge, LA 70803 USA

[3] Amer Univ, Washington, DC 20016 USA

[4] Univ Salerno, I-84084 Salerno, Italy

[5] Complesso Univ Monte S Angelo, INFN, Sez Napoli, I-80126 Naples, Italy

[6] Univ Florida, Gainesville, FL 32611 USA

[7] LIGO Livingston Observ, Livingston, LA 70754 USA

[8] Univ Savoie Mont Blanc, CNRS, IN2P3, Lab Annecy Le Vieux Phys Particules LAPP, F-74941 Annecy Le Vieux, France

[9] Univ Sannio Benevento, I-82100 Benevento, Italy

[10] INFN, Sez Napoli, I-80100 Naples, Italy

[11] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[12] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[13] MIT, LIGO, Cambridge, MA 02139 USA

[14] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil

[15] Gran Sasso Sci Inst, INFN, I-67100 Laquila, Italy

[16] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy

[17] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India

[18] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India

[19] Natl Astron Observ Japan, 2-21-1 Ohsawa, Mitaka, Tokyo 1818588, Japan

[20] Univ Wisconsin Milwaukee, Milwaukee, WI 53201 USA

[21] Leibniz Univ Hannover, D-30167 Hannover, Germany

[22] Univ Pisa, I-56127 Pisa, Italy

[23] INFN, Sez Pisa, I-56127 Pisa, Italy

[24] Australian Natl Univ, Canberra, ACT 0200, Australia

[25] Univ Tokyo, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[26] Univ Tokyo, Res Ctr Early Univ, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[27] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, 1-1-1 Yayoi, Tokyo 1130032, Japan

[28] Calif State Univ Fullerton, Fullerton, CA 92831 USA

[29] Univ Paris Saclay, Univ Paris Sud, CNRS, IN2P3,LAL, F-91898 Orsay, France

[30] Chennai Math Inst, Chennai 603103, Tamil Nadu, India

[31] Hirosaki Univ, Dept Adv Phys, 3 Bunkyo Cho, Hirosaki, Aomori 0368561, Japan

[32] Univ Roma Tor Vergata, I-00133 Rome, Italy

[33] Univ Hamburg, D-22761 Hamburg, Germany

[34] INFN, Sez Roma, I-00185 Rome, Italy

[35] Tokyo Inst Technol, Grad Sch Sci & Technol, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528551, Japan

[36] Univ Tokyo, Inst Cosm Ray Res, Higashi Mozumi 238,Kamioka Cho, Hida, Gifu 5061205, Japan

[37] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, Germany

[38] Univ Paris Diderot, CNRS IN2P3, CEA Irfu, Sorbonne Paris Cite,Observ Paris,APC, F-75205 Paris 13, France

[39] Osaka Univ, Grad Sch Sci, Phys, 1-1 Machikaneyama Cho, Toyonaka, Osaka 5600043, Japan

[40] West Virginia Univ, Morgantown, WV 26506 USA

[41] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Morgantown, WV 26505 USA

[42] Univ Perugia, I-06123 Perugia, Italy

[43] INFN, Sez Perugia, I-06123 Perugia, Italy

[44] EGO, I-56021 Pisa, Italy

[45] Syracuse Univ, Syracuse, NY 13244 USA

[46] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland

[47] LIGO Hanford Observ, Richland, WA 99352 USA

[48] RMKI, Wigner RCP, H-1121 Budapest, Hungary

[49] Columbia Univ, New York, NY 10027 USA

[50] Stanford Univ, Stanford, CA 94305 USA

来源：

LIVING REVIEWS IN RELATIVITY | 2018年 / 21卷

基金：

俄罗斯科学基金会; 瑞士国家科学基金会; 新加坡国家研究基金会; 澳大利亚研究理事会; 中国国家自然科学基金; 匈牙利科学研究基金会; 美国国家科学基金会; 俄罗斯基础研究基金会;

关键词：

Gravitational waves; Gravitational-wave detectors; Electromagnetic counterparts; Data analysis; BINARY NEUTRON-STAR; BLACK-HOLE MERGERS; GAMMA-RAY BURSTS; SWIFT FOLLOW-UP; ELECTROMAGNETIC SIGNALS; COMPACT BINARIES; EVENTS GW150914; SEARCH; COUNTERPART; ASSOCIATION;

D O I：

10.1007/s41114-018-0012-9

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5-20 deg(2) requires at least three detectors of sensitivity within a factor of similar to 2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.

引用

页数：57

共 299 条

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Biermann, P. L. ;

Billoir, P. ;

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Blaess, S. G. ;

Blanco, A. ;

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Bleve, C. ;

Bohacova, M. ;

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Bonifazi, C. ;

Borodai, N. ;

Botti, A. M. ;

Brack, J. ;

Brancus, I. ;

Bretz, T. ;

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← 1 2 3 4 5 6 7 8 9 10 →

共 299 条

[1] Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory [J].

Aab, A. ;

Abreu, P. ;

Aglietta, M. ;

Al Samarai, I. ;

Albuquerque, I. F. M. ;

Allekotte, I. ;

Almela, A. ;

Alvarez Castillo, J. ;

Alvarez-Muniz, J. ;

Ambrosio, M. ;

Anastasi, G. A. ;

Anchordoqui, L. ;

Andrada, B. ;

Andringa, S. ;

Aramo, C. ;

Arqueros, F. ;

Arsene, N. ;

Asorey, H. ;

Assis, P. ;

Aublin, J. ;

Avila, G. ;

Badescu, A. M. ;

Balaceanu, A. ;

Barreira Luz, R. J. ;

Baus, C. ;

Beatty, J. J. ;

Becker, K. H. ;

Bellido, J. A. ;

Berat, C. ;

Bertaina, M. E. ;

Bertou, X. ;

Biermann, P. L. ;

Billoir, P. ;

Biteau, J. ;

Blaess, S. G. ;

Blanco, A. ;

Blazek, J. ;

Bleve, C. ;

Bohacova, M. ;

Boncioli, D. ;

Bonifazi, C. ;

Borodai, N. ;

Botti, A. M. ;

Brack, J. ;

Brancus, I. ;

Bretz, T. ;

Bridgeman, A. ;

Briechle, F. L. ;

Buchholz, P. ;

Bueno, A. .

PHYSICAL REVIEW D, 2016, 94 (12)

[2] Characterization of the LIGO detectors during their sixth science run [J].

Aasi, J. ;

Abadie, J. ;

Abbott, B. P. ;

Abbott, R. ;

Abbott, T. ;

Abernathy, M. R. ;

Accadia, T. ;

Acernese, F. ;

Adams, C. ;

Adams, T. ;

Adhikari, R. X. ;

Affeldt, C. ;

Agathos, M. ;

Aggarwal, N. ;

Aguiar, O. D. ;

Ajith, P. ;

Allen, B. ;

Allocca, A. ;

Ceron, E. Amador ;

Amariutei, D. ;

Anderson, R. A. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arai, K. ;

Araya, M. C. ;

Arceneaux, C. ;

Areeda, J. ;

Ast, S. ;

Aston, S. M. ;

Astone, P. ;

Aufmuth, P. ;

Aulbert, C. ;

Austin, L. ;

Aylott, B. E. ;

Babak, S. ;

Baker, P. T. ;

Ballardin, G. ;

Ballmer, S. W. ;

Barayoga, J. C. ;

Barker, D. ;

Barnum, S. H. ;

Barone, F. ;

Barr, B. ;

Barsotti, L. ;

Barsuglia, M. ;

Barton, M. A. ;

Bartos, I. ;

Bassiri, R. ;

Basti, A. ;

Batch, J. .

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Aasi, J. ;

Abbott, B. P. ;

Abbott, R. ;

Abbott, T. ;

Abernathy, M. R. ;

Acernese, F. ;

Ackley, K. ;

Adams, C. ;

Adams, T. ;

Addesso, P. ;

Adhikari, R. X. ;

Affeldt, C. ;

Agathos, M. ;

Aggarwal, N. ;

Aguiar, O. D. ;

Ajith, P. ;

Alemic, A. ;

Allen, B. ;

Allocca, A. ;

Amariutei, D. ;

Andersen, M. ;

Anderson, R. A. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arai, K. ;

Araya, M. C. ;

Arceneaux, C. ;

Areeda, J. S. ;

Ast, S. ;

Aston, S. M. ;

Astone, P. ;

Aufmuth, P. ;

Augustus, H. ;

Aulbert, C. ;

Aylott, B. E. ;

Babak, S. ;

Baker, P. T. ;

Ballardin, G. ;

Ballmer, S. W. ;

Barayoga, J. C. ;

Barbet, M. ;

Barish, B. C. ;

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