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; C. P.L. Berry; C. Bond; W. Del Pozzo; W. M. Farr; A. Freise; A. C. Green; C. J. Haster; H. Middleton; C. M. Mow-Lowry; D. Töyrä; A. Vecchio; J. Veitch; S. Vinciguerra; W. D. Vousden; H. Wang; M. Wang; The 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, C. P.L. Berry, C. Bond, W. Del Pozzo, W. M. Farr, A. Freise, A. C. Green, C. J. Haster, H. Middleton, C. M. Mow-Lowry, D. Töyrä, A. Vecchio, J. Veitch, S. Vinciguerra, W. D. Vousden, H. Wang, M. Wang, The LIGO Scientific Collaboration

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

416 Citations (Scopus)

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
Article number	044001
Journal	Classical and Quantum Gravity
Volume	34
Issue number	4
DOIs	https://doi.org/10.1088/1361-6382/aa51f4
Publication status	Published - 24 Jan 2017

Keywords

cosmic explorer
gravitational waves
LIGO

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

Access to Document

10.1088/1361-6382/aa51f4Licence: None: All rights reserved

http://iopscience.iop.org/article/10.1088/1361-6382/aa51f4/metaLicence: None: All rights reserved

Birmingham Astrophysics : Consolidated Grant 2013-2016
Vecchio, A. (Principal Investigator), Ponman, T. (Co-Investigator), Freise, A. (Co-Investigator), Smith, G. (Co-Investigator), Speake, C. (Co-Investigator), Mandel, I. (Co-Investigator), Cruise, M. (Co-Investigator), Raychaudhury, S. (Co-Investigator) & Stevens, I. (Co-Investigator)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/13 → 30/09/16
Project: Research Councils
UK Involvement in the Operations of Advanced LIGO
Vecchio, A. (Principal Investigator) & Freise, A. (Co-Investigator)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/08/11 → 31/12/15
Project: Research Councils
UK Involvement in the Advanced LIGO Gravitational Wave Project
Vecchio, A. (Principal Investigator), Castelli, C. (Co-Investigator) & Cruise, M. (Co-Investigator)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/06/03 → 31/03/11
Project: Research Councils

Cite this

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., ... The 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

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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 = "cosmic explorer, gravitational waves, LIGO",

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 Berry, \{C. P.L.\} and C. Bond and \{Del Pozzo\}, W. and Farr, \{W. M.\} and A. Freise and Green, \{A. C.\} and Haster, \{C. J.\} and H. Middleton and Mow-Lowry, \{C. M.\} and D. T{\"o}yr{\"a} and A. Vecchio and J. Veitch and S. Vinciguerra and Vousden, \{W. D.\} and H. Wang and M. Wang and \{The LIGO Scientific Collaboration\}",

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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, Berry, CPL, Bond, C, Del Pozzo, W, Farr, WM, Freise, A, Green, AC, Haster, CJ, Middleton, H, Mow-Lowry, CM, Töyrä, D, Vecchio, A, Veitch, J, Vinciguerra, S, Vousden, WD, Wang, H, Wang, M & The 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

TY - JOUR

T1 - Exploring the sensitivity of next generation gravitational wave detectors

AU - Abbott, B. P.

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 - Berry, C. P.L.

AU - Bond, C.

AU - Del Pozzo, W.

AU - Farr, W. M.

AU - Freise, A.

AU - Green, A. C.

AU - Haster, C. J.

AU - Middleton, H.

AU - Mow-Lowry, C. M.

AU - Töyrä, D.

AU - Vecchio, A.

AU - Veitch, J.

AU - Vinciguerra, S.

AU - Vousden, W. D.

AU - Wang, H.

AU - Wang, M.

AU - The 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 - cosmic explorer

KW - gravitational waves

KW - LIGO

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

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

Keywords

ASJC Scopus subject areas

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Projects

Birmingham Astrophysics : Consolidated Grant 2013-2016

UK Involvement in the Operations of Advanced LIGO

UK Involvement in the Advanced LIGO Gravitational Wave Project

Cite this