Exploring the sensitivity of next generation gravitational wave detectors

被引:760
|
作者
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Abbott, T. D. [2 ]
Abernathy, M. R. [3 ]
Ackley, K. [4 ]
Adams, C. [5 ]
Addesso, P. [6 ,7 ]
Adhikari, R. X. [1 ]
Adya, V. B. [8 ]
Affeldt, C. [8 ]
Aggarwal, N. [9 ]
Aguiar, O. D. [10 ]
Ain, A. [11 ]
Ajith, P. [12 ]
Allen, B. [8 ,13 ,14 ]
Altin, P. A. [15 ]
Anderson, S. B. [1 ]
Anderson, W. G. [13 ]
Arai, K. [1 ]
Araya, M. C. [1 ]
Arceneaux, C. C. [16 ]
Areeda, J. S. [17 ]
Arun, K. G. [18 ]
Ashton, G.
Ast, M. [20 ]
Aston, S. M. [5 ,19 ]
Aufmuth, P. [14 ]
Aulbert, C. [8 ]
Babak, S. [21 ]
Baker, P. T. [22 ]
Ballmer, S. W. [23 ]
Barayoga, J. C. [1 ]
Barclay, S. E. [24 ]
Barish, B. C. [1 ]
Barker, D. [25 ]
Barr, B. [24 ]
Barsotti, L. [9 ]
Bartlett, J. [25 ]
Bartos, I. [26 ]
Bassiri, R. [27 ]
Batch, J. C. [25 ]
Baune, C. [8 ]
Bell, A. S. [24 ]
Berger, B. K. [1 ]
Bergmann, G. [8 ]
Berry, C. P. L. [28 ]
Betzwieser, J. [5 ]
Bhagwat, S. [23 ]
Bhandare, R. [29 ]
Bilenko, I. A. [30 ]
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 Florida, Gainesville, FL 32611 USA
[5] LIGO Livingston Observ, Livingston, LA 70754 USA
[6] Univ Sannio Benevento, I-82100 Benevento, Italy
[7] INFN, Sez Napoli, I-80100 Naples, Italy
[8] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[9] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[10] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, Brazil
[11] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[12] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560012, Karnataka, India
[13] Univ Wisconsin, Milwaukee, WI 53201 USA
[14] Leibniz Univ Hannover, D-30167 Hannover, Germany
[15] Australian Natl Univ, Canberra, ACT 0200, Australia
[16] Univ Mississippi, University, MS 38677 USA
[17] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[18] Chennai Math Inst, Madras 603103, Tamil Nadu, India
[19] Univ Southampton, Southampton SO17 1BJ, Hants, England
[20] Univ Hamburg, D-22761 Hamburg, Germany
[21] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[22] Montana State Univ, Bozeman, MT 59717 USA
[23] Syracuse Univ, Syracuse, NY 13244 USA
[24] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland
[25] LIGO Hanford Observ, Richland, WA 99352 USA
[26] Columbia Univ, New York, NY 10027 USA
[27] Stanford Univ, Stanford, CA 94305 USA
[28] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[29] RRCAT, Indore 452013, Madhya Pradesh, India
[30] Lomonosov Moscow State Univ, Fac Phys, Moscow 119991, Russia
[31] Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland
[32] Univ Western Australia, Crawley, WA 6009, Australia
[33] Washington State Univ, Pullman, WA 99164 USA
[34] Univ Oregon, Eugene, OR 97403 USA
[35] Carleton Coll, Northfield, MN 55057 USA
[36] Univ Maryland, College Pk, MD 20742 USA
[37] Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA
[38] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA
[39] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[40] Univ Tokyo, RESCEU, Tokyo 1130033, Japan
[41] Tsinghua Univ, Beijing 100084, Peoples R China
[42] Texas Tech Univ, Lubbock, TX 79409 USA
[43] Penn State Univ, University Pk, PA 16802 USA
[44] Natl Tsing Hua Univ, Hsinchu 30013, Taiwan
[45] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia
[46] West Virginia Univ, Morgantown, WV 26506 USA
[47] Univ Chicago, Chicago, IL 60637 USA
[48] CALTECH, CaRT, Pasadena, CA 91125 USA
[49] Korea Inst Sci & Technol Informat, Daejeon 305806, South Korea
[50] Univ Brussels, B-1050 Brussels, Belgium
基金
美国国家科学基金会;
关键词
gravitational waves; cosmic explorer; LIGO; SQUEEZED VACUUM STATES; QUANTUM OPTICS; NOISE;
D O I
10.1088/1361-6382/aa51f4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.
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页数:18
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