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 › Academic › peer-review

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
Number of pages	18
Journal	Classical and Quantum Gravity
Volume	34
Issue number	4
DOIs	https://doi.org/10.1088/1361-6382/aa51f4
Publication status	Published - 23 Feb 2017
Externally published	Yes

Keywords

gravitational waves
cosmic explorer
LIGO
SQUEEZED VACUUM STATES
QUANTUM OPTICS
NOISE

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10.1088/1361-6382/aa51f4Licence: Other

https://digital.library.adelaide.edu.au/dspace/bitstream/2440/116533/4/hdl_116533.pdfLicence: CC BY-NC-ND

Cite this

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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 = "gravitational waves, cosmic explorer, LIGO, SQUEEZED VACUUM STATES, QUANTUM OPTICS, NOISE",

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

year = "2017",

month = feb,

day = "23",

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

language = "English",

volume = "34",

journal = "Classical and Quantum Gravity",

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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 - 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 - Danilishin, S.L.

AU - Hennig, J.

AU - Hild, S.

AU - Steinlechner, J.

AU - Steinlechner, S.

AU - LIGO Scientific Collaboration

PY - 2017/2/23

Y1 - 2017/2/23

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 - gravitational waves

KW - cosmic explorer

KW - LIGO

KW - SQUEEZED VACUUM STATES

KW - QUANTUM OPTICS

KW - NOISE

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

Keywords

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