Exploring the sensitivity of next generation gravitational wave detectors

B. P. Abbott; R. Abbott; T. D. Abbott; M. R. Abernathy; K. Ackley; C. Adams; P. Addesso; R. X. Adhikari; V. B. Adya; C. Affeldt; N. Aggarwal; O. D. Aguiar; A. Ain; P. Ajith; B. Allen; P. A. Altin; S. B. Anderson; W. G. Anderson; K. Arai; M. C. Araya; C. C. Arceneaux; J. S. Areeda; K. G. Arun; G. Ashton; M. Ast; S. M. Aston; P. Aufmuth; C. Aulbert; S. Babak; P. T. Baker; S. W. Ballmer; J. C. Barayoga; S. E. Barclay; B. C. Barish; D. Barker; B. Barr; L. Barsotti; J. Bartlett; I. Bartos; R. Bassiri; J. C. Batch; C. Baune; A. S. Bell; B. K. Berger; G. Bergmann; C. P L Berry; J. Betzwieser; S. Bhagwat; R. Bhandare; V. Mandic; ligo Scientific Collaboration

doi:10.1088/1361-6382/aa51f4

Exploring the sensitivity of next generation gravitational wave detectors

B. P. Abbott
, R. Abbott
, T. D. Abbott
, M. R. Abernathy
, K. Ackley
, C. Adams
, P. Addesso
, R. X. Adhikari
, V. B. Adya
, C. Affeldt
, N. Aggarwal
, O. D. Aguiar
, A. Ain
, P. Ajith
, B. Allen
, P. A. Altin
, S. B. Anderson
, W. G. Anderson
, K. Arai
, M. C. Araya

C. C. Arceneaux, J. S. Areeda, K. G. Arun, G. Ashton, M. Ast, S. M. Aston, P. Aufmuth, C. Aulbert, S. Babak, P. T. Baker, S. W. Ballmer, J. C. Barayoga, S. E. Barclay, B. C. Barish, D. Barker, B. Barr, L. Barsotti, J. Bartlett, I. Bartos, R. Bassiri, J. C. Batch, C. Baune, A. S. Bell, B. K. Berger, G. Bergmann, C. P L Berry, J. Betzwieser, S. Bhagwat, R. Bhandare, V. Mandic, ligo Scientific Collaboration

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

1090 Scopus citations

Abstract

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.

Original language	English (US)
Article number	044001
Journal	Classical and Quantum Gravity
Volume	34
Issue number	4
DOIs	https://doi.org/10.1088/1361-6382/aa51f4
State	Published - Jan 24 2017

Bibliographical note

Publisher Copyright:
© 2017 IOP Publishing Ltd.

Keywords

LIGO
cosmic explorer
gravitational waves

Publisher link

10.1088/1361-6382/aa51f4

http://hdl.handle.net/2440/116533

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Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Ackley, K., Adams, C., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Aggarwal, N., Aguiar, O. D., Ain, A., Ajith, P., Allen, B., Altin, P. A., Anderson, S. B., Anderson, W. G., Arai, K., ... ligo Scientific Collaboration (2017). Exploring the sensitivity of next generation gravitational wave detectors. Classical and Quantum Gravity, 34(4), Article 044001. https://doi.org/10.1088/1361-6382/aa51f4

Abbott, BP, Abbott, R, Abbott, TD, Abernathy, MR, Ackley, K, Adams, C, Addesso, P, Adhikari, RX, Adya, VB, Affeldt, C, Aggarwal, N, Aguiar, OD, Ain, A, Ajith, P, Allen, B, Altin, PA, Anderson, SB, Anderson, WG, Arai, K, Araya, MC, Arceneaux, CC, Areeda, JS, Arun, KG, Ashton, G, Ast, M, Aston, SM, Aufmuth, P, Aulbert, C, Babak, S, Baker, PT, Ballmer, SW, Barayoga, JC, Barclay, SE, Barish, BC, Barker, D, Barr, B, Barsotti, L, Bartlett, J, Bartos, I, Bassiri, R, Batch, JC, Baune, C, Bell, AS, Berger, BK, Bergmann, G, Berry, CPL, Betzwieser, J, Bhagwat, S, Bhandare, R, Mandic, V & ligo Scientific Collaboration 2017, 'Exploring the sensitivity of next generation gravitational wave detectors', Classical and Quantum Gravity, vol. 34, no. 4, 044001. https://doi.org/10.1088/1361-6382/aa51f4

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abstract = "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.",

keywords = "LIGO, cosmic explorer, gravitational waves",

author = "Abbott, \{B. P.\} and R. Abbott and Abbott, \{T. D.\} and Abernathy, \{M. R.\} and K. Ackley and C. Adams and P. Addesso and Adhikari, \{R. X.\} and Adya, \{V. B.\} and C. Affeldt and N. Aggarwal and Aguiar, \{O. D.\} and A. Ain and P. Ajith and B. Allen and Altin, \{P. A.\} and Anderson, \{S. B.\} and Anderson, \{W. G.\} and K. Arai and Araya, \{M. C.\} and Arceneaux, \{C. C.\} and Areeda, \{J. S.\} and Arun, \{K. G.\} and G. Ashton and M. Ast and Aston, \{S. M.\} and P. Aufmuth and C. Aulbert and S. Babak and Baker, \{P. T.\} and Ballmer, \{S. W.\} and Barayoga, \{J. C.\} and Barclay, \{S. E.\} and Barish, \{B. C.\} and D. Barker and B. Barr and L. Barsotti and J. Bartlett and I. Bartos and R. Bassiri and Batch, \{J. C.\} and C. Baune and Bell, \{A. S.\} and Berger, \{B. K.\} and G. Bergmann and Berry, \{C. P L\} and J. Betzwieser and S. Bhagwat and R. Bhandare and V. Mandic and \{ligo Scientific Collaboration\}",

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AU - Abbott, R.

AU - Abbott, T. D.

AU - Abernathy, M. R.

AU - Ackley, K.

AU - Adams, C.

AU - Addesso, P.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Ain, A.

AU - Ajith, P.

AU - Allen, B.

AU - Altin, P. A.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Arai, K.

AU - Araya, M. C.

AU - Arceneaux, C. C.

AU - Areeda, J. S.

AU - Arun, K. G.

AU - Ashton, G.

AU - Ast, M.

AU - Aston, S. M.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - Babak, S.

AU - Baker, P. T.

AU - Ballmer, S. W.

AU - Barayoga, J. C.

AU - Barclay, S. E.

AU - Barish, B. C.

AU - Barker, D.

AU - Barr, B.

AU - Barsotti, L.

AU - Bartlett, J.

AU - Bartos, I.

AU - Bassiri, R.

AU - Batch, J. C.

AU - Baune, C.

AU - Bell, A. S.

AU - Berger, B. K.

AU - Bergmann, G.

AU - Berry, C. P L

AU - Betzwieser, J.

AU - Bhagwat, S.

AU - Bhandare, R.

AU - Mandic, V.

AU - ligo Scientific Collaboration

PY - 2017/1/24

Y1 - 2017/1/24

N2 - 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.

AB - 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.

KW - LIGO

KW - cosmic explorer

KW - gravitational waves

UR - https://www.scopus.com/pages/publications/85011982160

UR - https://www.scopus.com/pages/publications/85011982160#tab=citedBy

U2 - 10.1088/1361-6382/aa51f4

DO - 10.1088/1361-6382/aa51f4

M3 - Article

AN - SCOPUS:85011982160

SN - 0264-9381

VL - 34

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 4

M1 - 044001

ER -

Exploring the sensitivity of next generation gravitational wave detectors

Abstract

Bibliographical note

Keywords

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