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

[91]

[Anonymous], CQGRA

[92] Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger [J].

Arcavi, Iair ;

Hosseinzadeh, Griffin ;

Howell, D. Andrew ;

McCully, Curtis ;

Poznanski, Dovi ;

Kasen, Daniel ;

Barnes, Jennifer ;

Zaltzman, Michael ;

Vasylyev, Sergiy ;

Maoz, Dan ;

Valenti, Stefano .

NATURE, 2017, 551 (7678) :64-+

[93] Optical Follow-up of Gravitational-wave Events with Las Cumbres Observatory [J].

Arcavi, Iair ;

McCully, Curtis ;

Hosseinzadeh, Griffin ;

Howell, D. Andrew ;

Vasylyev, Sergiy ;

Poznanski, Dovi ;

Zaltzman, Michael ;

Maoz, Dan ;

Singer, Leo ;

Valenti, Stefano ;

Kasen, Daniel ;

Barnes, Jennifer ;

Piran, Tsvi ;

Fong, Wen-fai .

ASTROPHYSICAL JOURNAL LETTERS, 2017, 848 (02)

[94] Interferometer design of the KAGRA gravitational wave detector [J].

Aso, Yoichi ;

Michimura, Yuta ;

Somiya, Kentaro ;

Ando, Masaki ;

Miyakawa, Osamu ;

Sekiguchi, Takanori ;

Tatsumi, Daisuke ;

Yamamoto, Hiroaki .

PHYSICAL REVIEW D, 2013, 88 (04)

[95] A template bank to search for gravitational waves from inspiralling compact binaries: I. Physical models [J].

Babak, S. ;

Balasubramanian, R. ;

Churches, D. ;

Cokelaer, T. ;

Sathyaprakash, B. S. .

CLASSICAL AND QUANTUM GRAVITY, 2006, 23 (18) :5477-5504

[96] Searching for gravitational waves from binary coalescence [J].

Babak, S. ;

Biswas, R. ;

Brady, P. R. ;

Brown, D. A. ;

Cannon, K. ;

Capano, C. D. ;

Clayton, J. H. ;

Cokelaer, T. ;

Creighton, J. D. E. ;

Dent, T. ;

Dietz, A. ;

Fairhurst, S. ;

Fotopoulos, N. ;

Gonzalez, G. ;

Hanna, C. ;

Harry, I. W. ;

Jones, G. ;

Keppel, D. ;

McKechan, D. J. A. ;

Pekowsky, L. ;

Privitera, S. ;

Robinson, C. ;

Rodriguez, A. C. ;

Sathyaprakash, B. S. ;

Sengupta, A. S. ;

Vallisneri, M. ;

Vaulin, R. ;

Weinstein, A. J. .

PHYSICAL REVIEW D, 2013, 87 (02)

[97] Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO [J].

Bagoly, Zsolt ;

Szecsi, Dorottya ;

Balazs, Lajos G. ;

Csabai, Istvan ;

Horvath, Istvan ;

Dobos, Laszlo ;

Lichtenberger, Janos ;

Toth, L. Viktor .

ASTRONOMY & ASTROPHYSICS, 2016, 593

[98] Strong Constraints on Cosmological Gravity from GW170817 and GRB 170817A [J].

Baker, T. ;

Bellini, E. ;

Ferreira, P. G. ;

Lagos, M. ;

Noller, J. ;

Sawicki, I. .

PHYSICAL REVIEW LETTERS, 2017, 119 (25)

[99] Theory-Agnostic Constraints on Black-Hole Dipole Radiation with Multiband Gravitational-Wave Astrophysics [J].

Barausse, Enrico ;

Yunes, Nicolas ;

Chamberlain, Katie .

PHYSICAL REVIEW LETTERS, 2016, 116 (24)

[100] Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei [J].

Bartos, Imre ;

Kocsis, Bence ;

Haiman, Zoltan ;

Marka, Szabolcs .

ASTROPHYSICAL JOURNAL, 2017, 835 (02)

← 5 6 7 8 9 10 11 12 13 14 →