Exploring the sensitivity of next generation gravitational wave detectors

LIGO Scientific Collaboration

doi:10.1088/1361-6382/aa51f4

Exploring the sensitivity of next generation gravitational wave detectors

LIGO Scientific Collaboration

Physics and Astronomy

Research output: Contribution to journal › Article

288 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
Article number	044001
Journal	Classical and Quantum Gravity
Volume	34
Issue number	4
DOIs	https://doi.org/10.1088/1361-6382/aa51f4
State	Published - 24 Jan 2017

Keywords

LIGO
cosmic explorer
gravitational waves

Access to Document

10.1088/1361-6382/aa51f4

Link to publication in Scopus

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LIGO Scientific Collaboration (2017). Exploring the sensitivity of next generation gravitational wave detectors. Classical and Quantum Gravity, 34(4), [044001]. https://doi.org/10.1088/1361-6382/aa51f4

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title = "Exploring the sensitivity of next generation gravitational wave detectors",

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 = "{LIGO Scientific Collaboration} and 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 Bilenko, {I. A.}",

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AU - LIGO Scientific Collaboration

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 - 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 - Bilenko, I. A.

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

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