Exploring the sensitivity of next generation gravitational wave detectors

被引：913

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

来源：

CLASSICAL AND QUANTUM GRAVITY | 2017年 / 34卷 / 04期

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.

引用

页数：18

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