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

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

1050 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

All Science Journal Classification (ASJC) codes

Physics and Astronomy (miscellaneous)

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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.",

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 C. Hanna and Sathyaprakash, \{B. S.\}",

year = "2017",

month = jan,

day = "24",

doi = "10.1088/1361-6382/aa51f4",

language = "English (US)",

volume = "34",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "4",

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TY - JOUR

T1 - Exploring the sensitivity of next generation gravitational wave detectors

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 - Hanna, C.

AU - Sathyaprakash, B. S.

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.

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

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

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