Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo

被引：247

作者：

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

Abbott, R. ^{[1
]}

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

Abernathy, M. R. ^{[1
]}

Acernese, F. ^{[3
,4
]}

Ackley, K. ^{[5
]}

Adams, C. ^{[6
]}

Adams, T. ^{[7
]}

Addesso, P. ^{[8
,9
]}

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

Adya, V. B. ^{[10
]}

Affeldt, C. ^{[10
]}

Agathos, M. ^{[11
]}

Agatsuma, K. ^{[11
]}

Aggarwal, N. ^{[12
]}

Aguiar, O. D. ^{[13
]}

Ain, A. ^{[14
]}

Ajith, P. ^{[15
]}

Allen, B. ^{[10
,16
,17
]}

Allocca, A. ^{[18
,19
]}

Altin, P. A. ^{[20
]}

Amariutei, D. V. ^{[5
]}

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

Anderson, W. G. ^{[16
]}

Arai, K. ^{[1
]}

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

Arceneaux, C. C. ^{[21
]}

Areeda, J. S. ^{[22
]}

Arnaud, N. ^{[23
]}

Arun, K. G. ^{[24
]}

Ashton, G. ^{[25
]}

Ast, M. ^{[26
]}

Aston, S. M. ^{[6
]}

Astone, P. ^{[27
]}

Aufmuth, P. ^{[17
]}

Aulbert, C. ^{[10
]}

Babak, S. ^{[28
]}

Baker, P. T. ^{[29
]}

Baldaccini, F. ^{[30
,31
]}

Ballardin, G. ^{[32
]}

Ballmer, S. W. ^{[33
]}

Barayoga, J. C. ^{[1
]}

Barclay, S. E. ^{[34
]}

Barish, B. C. ^{[1
]}

Barker, D. ^{[35
]}

Barone, F. ^{[3
,4
]}

Barr, B. ^{[34
]}

Barsotti, L. ^{[12
]}

Barsuglia, M. ^{[36
]}

Barta, D. ^{[37
]}

机构：

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

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

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

[4] Complesso Univ Monte S Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

[5] Univ Florida, Gainesville, FL 32611 USA

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

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

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

[9] Ist Nazl Fis Nucl, Sez Napoli, I-80100 Naples, Italy

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

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

[12] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA

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

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

[15] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560012, Karnataka, India

[16] Univ Wisconsin, Milwaukee, WI 53201 USA

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

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

[19] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[20] Australian Natl Univ, GPO Box 4, Canberra, ACT 0200, Australia

[21] Univ Mississippi, University, MS 38677 USA

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

[23] Univ Paris Saclay, Univ Paris 11, CNRS IN2P3, LAL, Orsay, France

[24] Chennai Math Inst, Madras, Tamil Nadu, India

[25] Univ Southampton, Southampton SO17 1BJ, Hants, England

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

[27] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy

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

[29] Montana State Univ, Bozeman, MT 59717 USA

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

[31] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[32] EGO, I-56021 Pisa, Italy

[33] Syracuse Univ, Syracuse, NY 13244 USA

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

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

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

[37] RMKI, Wigner RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary

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

[39] Stanford Univ, Stanford, CA 94305 USA

[40] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy

[41] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[42] CAMK PAN, PL-00716 Warsaw, Poland

[43] Warsaw Univ, Astron Observ, PL-00478 Warsaw, Poland

[44] Univ Birmingham, Birmingham B15 2TT, W Midlands, England

[45] Univ Genoa, I-16146 Genoa, Italy

[46] Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[47] RRCAT, Indore 452013, MP, India

[48] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia

[49] Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland

[50] Univ Western Australia, Crawley, WA 6009, Australia

来源：

LIVING REVIEWS IN RELATIVITY | 2016年 / 19卷

基金：

新加坡国家研究基金会; 澳大利亚研究理事会; 美国国家科学基金会; 英国科学技术设施理事会;

关键词：

Gravitational waves; Gravitational-wave detectors; Electromagnetic counterparts; Data analysis; FOLLOW-UP; PARAMETER-ESTIMATION; BINARY INSPIRALS; SEARCH; COUNTERPARTS; RADIATION; MERGERS; BURSTS;

D O I：

10.1007/lrr-2016-1

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 a possible observing scenario for the Advanced LIGO and Advanced Virgo 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 determine the expected 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 considered the most promising 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 deg(2) to 20 deg(2) will require at least three detectors of sensitivity within a factor of similar to 2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.

引用

页码：1 / 39

页数：39

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