The Einstein Telescope: a third-generation gravitational wave observatory

M. Punturo; M. Abernathy; F. Acernese; B. Allen; N. Andersson; K. Arun; F. Barone; B. Barr; M. Barsuglia; M. Beker; N. Beveridge; S. Birindelli; S. Bose; L. Bosi; S. Braccini; C. Bradaschia; T. Bulik; E. Calloni; G. Cella; E.C. Mottin; S. Chelkowski; A. Chincarini; J. Clark; E. Coccia; C. Colacino; J. Colas; A. Cumming; L. Cunningham; E. Cuoco; S. Danilishin; K. Danzmann; G. De Luca; R. De Salvo; T. Dent; R. De Rosa; L. Di Fiore; A. Di Virgilio; M. Doets; V. Fafone; P. Falferi; R. Flaminio; J. Franc; F. Frasconi; A. Freise; P. Fulda; J. Gair; G. Gemme; A. Gennai; A. Giazotto; K. Glampedakis; S. Hild; J. van den Brand

doi:10.1088/0264-9381/27/19/194002

The Einstein Telescope: a third-generation gravitational wave observatory

M. Punturo^*, M. Abernathy, F. Acernese, B. Allen, N. Andersson, K. Arun, F. Barone, B. Barr, M. Barsuglia, M. Beker, N. Beveridge, S. Birindelli, S. Bose, L. Bosi, S. Braccini, C. Bradaschia, T. Bulik, E. Calloni, G. Cella, E.C. MottinS. Chelkowski, A. Chincarini, J. Clark, E. Coccia, C. Colacino, J. Colas, A. Cumming, L. Cunningham, E. Cuoco, S. Danilishin, K. Danzmann, G. De Luca, R. De Salvo, T. Dent, R. De Rosa, L. Di Fiore, A. Di Virgilio, M. Doets, V. Fafone, P. Falferi, R. Flaminio, J. Franc, F. Frasconi, A. Freise, P. Fulda, J. Gair, G. Gemme, A. Gennai, A. Giazotto, K. Glampedakis, S. Hild, J. van den Brand

^*Corresponding author for this work

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

1019 Citations (Web of Science)

Abstract

Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources'' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase.

Original language	English
Article number	194002
Number of pages	12
Journal	Classical and Quantum Gravity
Volume	27
Issue number	19
DOIs	https://doi.org/10.1088/0264-9381/27/19/194002
Publication status	Published - 7 Oct 2010
Externally published	Yes

Keywords

VIRGO INTERFEROMETER
NOISE
SUPERATTENUATOR
FIBER

Access to Document

10.1088/0264-9381/27/19/194002

Cite this

Punturo, M., Abernathy, M., Acernese, F., Allen, B., Andersson, N., Arun, K., Barone, F., Barr, B., Barsuglia, M., Beker, M., Beveridge, N., Birindelli, S., Bose, S., Bosi, L., Braccini, S., Bradaschia, C., Bulik, T., Calloni, E., Cella, G., ... van den Brand, J. (2010). The Einstein Telescope: a third-generation gravitational wave observatory. Classical and Quantum Gravity, 27(19), Article 194002. https://doi.org/10.1088/0264-9381/27/19/194002

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abstract = "Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources'' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase.",

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author = "M. Punturo and M. Abernathy and F. Acernese and B. Allen and N. Andersson and K. Arun and F. Barone and B. Barr and M. Barsuglia and M. Beker and N. Beveridge and S. Birindelli and S. Bose and L. Bosi and S. Braccini and C. Bradaschia and T. Bulik and E. Calloni and G. Cella and E.C. Mottin and S. Chelkowski and A. Chincarini and J. Clark and E. Coccia and C. Colacino and J. Colas and A. Cumming and L. Cunningham and E. Cuoco and S. Danilishin and K. Danzmann and {De Luca}, G. and {De Salvo}, R. and T. Dent and {De Rosa}, R. and {Di Fiore}, L. and {Di Virgilio}, A. and M. Doets and V. Fafone and P. Falferi and R. Flaminio and J. Franc and F. Frasconi and A. Freise and P. Fulda and J. Gair and G. Gemme and A. Gennai and A. Giazotto and K. Glampedakis and S. Hild and {van den Brand}, J.",

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Punturo, M, Abernathy, M, Acernese, F, Allen, B, Andersson, N, Arun, K, Barone, F, Barr, B, Barsuglia, M, Beker, M, Beveridge, N, Birindelli, S, Bose, S, Bosi, L, Braccini, S, Bradaschia, C, Bulik, T, Calloni, E, Cella, G, Mottin, EC, Chelkowski, S, Chincarini, A, Clark, J, Coccia, E, Colacino, C, Colas, J, Cumming, A, Cunningham, L, Cuoco, E, Danilishin, S, Danzmann, K, De Luca, G, De Salvo, R, Dent, T, De Rosa, R, Di Fiore, L, Di Virgilio, A, Doets, M, Fafone, V, Falferi, P, Flaminio, R, Franc, J, Frasconi, F, Freise, A, Fulda, P, Gair, J, Gemme, G, Gennai, A, Giazotto, A, Glampedakis, K, Hild, S & van den Brand, J 2010, 'The Einstein Telescope: a third-generation gravitational wave observatory', Classical and Quantum Gravity, vol. 27, no. 19, 194002. https://doi.org/10.1088/0264-9381/27/19/194002

TY - JOUR

T1 - The Einstein Telescope: a third-generation gravitational wave observatory

AU - Punturo, M.

AU - Abernathy, M.

AU - Acernese, F.

AU - Allen, B.

AU - Andersson, N.

AU - Arun, K.

AU - Barone, F.

AU - Barr, B.

AU - Barsuglia, M.

AU - Beker, M.

AU - Beveridge, N.

AU - Birindelli, S.

AU - Bose, S.

AU - Bosi, L.

AU - Braccini, S.

AU - Bradaschia, C.

AU - Bulik, T.

AU - Calloni, E.

AU - Cella, G.

AU - Mottin, E.C.

AU - Chelkowski, S.

AU - Chincarini, A.

AU - Clark, J.

AU - Coccia, E.

AU - Colacino, C.

AU - Colas, J.

AU - Cumming, A.

AU - Cunningham, L.

AU - Cuoco, E.

AU - Danilishin, S.

AU - Danzmann, K.

AU - De Luca, G.

AU - De Salvo, R.

AU - Dent, T.

AU - De Rosa, R.

AU - Di Fiore, L.

AU - Di Virgilio, A.

AU - Doets, M.

AU - Fafone, V.

AU - Falferi, P.

AU - Flaminio, R.

AU - Franc, J.

AU - Frasconi, F.

AU - Freise, A.

AU - Fulda, P.

AU - Gair, J.

AU - Gemme, G.

AU - Gennai, A.

AU - Giazotto, A.

AU - Glampedakis, K.

AU - Hild, S.

AU - van den Brand, J.

PY - 2010/10/7

Y1 - 2010/10/7

N2 - Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources'' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase.

AB - Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational wave observatories could permit detailed measurements of the sources'' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progress of the ET project which is currently in its design study phase.

KW - VIRGO INTERFEROMETER

KW - NOISE

KW - SUPERATTENUATOR

KW - FIBER

U2 - 10.1088/0264-9381/27/19/194002

DO - 10.1088/0264-9381/27/19/194002

M3 - Article

SN - 0264-9381

VL - 27

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 19

M1 - 194002

ER -