The third generation of gravitational wave observatories and their science reach

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. Chassande 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. Derosa; 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; M. Granata; H. Grote; G. Guidi; G. Hammond; M. Hannam; J. Harms; D. Heinert; M. Hendry; I. Heng; E. Hennes; S. Hild; J. Hough; S. Husa; S. Huttner; G. Jones; F. Khalili; K. Kokeyama; K. Kokkotas; B. Krishnan; M. Lorenzini; H. Lück; E. Majorana; I. Mandel; V. Mandic; I. Martin; C. Michel; Y. Minenkov; N. Morgado; S. Mosca; B. Mours; H. Müller-Ebhardt; P. Murray; R. Nawrodt; J. Nelson; R. Oshaughnessy; C. D. Ott; C. Palomba; A. Paoli; G. Parguez; A. Pasqualetti; R. Passaquieti; D. Passuello; L. Pinard; R. Poggiani; P. Popolizio; M. Prato; P. Puppo; D. Rabeling; P. Rapagnani; J. Read; T. Regimbau; H. Rehbein; S. Reid; L. Rezzolla; F. Ricci; F. Richard; A. Rocchi; S. Rowan; A. Rüdiger; B. Sassolas; B. Sathyaprakash; R. Schnabel; C. Schwarz; P. Seidel; A. Sintes; K. Somiya; F. Speirits; K. Strain; S. Strigin; P. Sutton; S. Tarabrin; J. Van Den Brand; C. Van Leewen; M. Van Veggel; C. Van Den Broeck; A. Vecchio; J. Veitch; F. Vetrano; A. Vicere; S. Vyatchanin; B. Willke; G. Woan; P. Wolfango; K. Yamamoto

doi:10.1088/0264-9381/27/8/084007

The third generation of gravitational wave observatories and their science reach

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. Chassande 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. Derosa, 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, M. Granata, H. Grote, G. Guidi, G. Hammond, M. Hannam, J. Harms, D. Heinert, M. Hendry, I. Heng, E. Hennes, S. Hild, J. Hough, S. Husa, S. Huttner, G. Jones, F. Khalili, K. Kokeyama, K. Kokkotas, B. Krishnan, M. Lorenzini, H. Lück, E. Majorana, I. Mandel, V. Mandic, I. Martin, C. Michel, Y. Minenkov, N. Morgado, S. Mosca, B. Mours, H. Müller-Ebhardt, P. Murray, R. Nawrodt, J. Nelson, R. Oshaughnessy, C. D. Ott, C. Palomba, A. Paoli, G. Parguez, A. Pasqualetti, R. Passaquieti, D. Passuello, L. Pinard, R. Poggiani, P. Popolizio, M. Prato, P. Puppo, D. Rabeling, P. Rapagnani, J. Read, T. Regimbau, H. Rehbein, S. Reid, L. Rezzolla, F. Ricci, F. Richard, A. Rocchi, S. Rowan, A. Rüdiger, B. Sassolas, B. Sathyaprakash, R. Schnabel, C. Schwarz, P. Seidel, A. Sintes, K. Somiya, F. Speirits, K. Strain, S. Strigin, P. Sutton, S. Tarabrin, J. Van Den Brand, C. Van Leewen, M. Van Veggel, C. Van Den Broeck, A. Vecchio, J. Veitch, F. Vetrano, A. Vicere, S. Vyatchanin, B. Willke, G. Woan, P. Wolfango, K. Yamamoto

Physics and Astronomy (Twin Cities)

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342 Scopus citations

Abstract

Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported.

Original language	English (US)
Article number	084007
Journal	Classical and Quantum Gravity
Volume	27
Issue number	8
DOIs	https://doi.org/10.1088/0264-9381/27/8/084007
State	Published - 2010

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10.1088/0264-9381/27/8/084007

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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., ... Yamamoto, K. (2010). The third generation of gravitational wave observatories and their science reach. Classical and Quantum Gravity, 27(8), Article 084007. https://doi.org/10.1088/0264-9381/27/8/084007

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, Chassande Mottin, E, 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, Derosa, R, Fiore, LD, Virgilio, AD, 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, Granata, M, Grote, H, Guidi, G, Hammond, G, Hannam, M, Harms, J, Heinert, D, Hendry, M, Heng, I, Hennes, E, Hild, S, Hough, J, Husa, S, Huttner, S, Jones, G, Khalili, F, Kokeyama, K, Kokkotas, K, Krishnan, B, Lorenzini, M, Lück, H, Majorana, E, Mandel, I, Mandic, V, Martin, I, Michel, C, Minenkov, Y, Morgado, N, Mosca, S, Mours, B, Müller-Ebhardt, H, Murray, P, Nawrodt, R, Nelson, J, Oshaughnessy, R, Ott, CD, Palomba, C, Paoli, A, Parguez, G, Pasqualetti, A, Passaquieti, R, Passuello, D, Pinard, L, Poggiani, R, Popolizio, P, Prato, M, Puppo, P, Rabeling, D, Rapagnani, P, Read, J, Regimbau, T, Rehbein, H, Reid, S, Rezzolla, L, Ricci, F, Richard, F, Rocchi, A, Rowan, S, Rüdiger, A, Sassolas, B, Sathyaprakash, B, Schnabel, R, Schwarz, C, Seidel, P, Sintes, A, Somiya, K, Speirits, F, Strain, K, Strigin, S, Sutton, P, Tarabrin, S, Van Den Brand, J, Van Leewen, C, Van Veggel, M, Van Den Broeck, C, Vecchio, A, Veitch, J, Vetrano, F, Vicere, A, Vyatchanin, S, Willke, B, Woan, G, Wolfango, P & Yamamoto, K 2010, 'The third generation of gravitational wave observatories and their science reach', Classical and Quantum Gravity, vol. 27, no. 8, 084007. https://doi.org/10.1088/0264-9381/27/8/084007

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abstract = "Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported.",

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doi = "10.1088/0264-9381/27/8/084007",

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volume = "27",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

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TY - JOUR

T1 - The third generation of gravitational wave observatories and their science reach

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 - Chassande Mottin, E.

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 - Derosa, R.

AU - Fiore, L. Di

AU - Virgilio, A. Di

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 - Granata, M.

AU - Grote, H.

AU - Guidi, G.

AU - Hammond, G.

AU - Hannam, M.

AU - Harms, J.

AU - Heinert, D.

AU - Hendry, M.

AU - Heng, I.

AU - Hennes, E.

AU - Hild, S.

AU - Hough, J.

AU - Husa, S.

AU - Huttner, S.

AU - Jones, G.

AU - Khalili, F.

AU - Kokeyama, K.

AU - Kokkotas, K.

AU - Krishnan, B.

AU - Lorenzini, M.

AU - Lück, H.

AU - Majorana, E.

AU - Mandel, I.

AU - Mandic, V.

AU - Martin, I.

AU - Michel, C.

AU - Minenkov, Y.

AU - Morgado, N.

AU - Mosca, S.

AU - Mours, B.

AU - Müller-Ebhardt, H.

AU - Murray, P.

AU - Nawrodt, R.

AU - Nelson, J.

AU - Oshaughnessy, R.

AU - Ott, C. D.

AU - Palomba, C.

AU - Paoli, A.

AU - Parguez, G.

AU - Pasqualetti, A.

AU - Passaquieti, R.

AU - Passuello, D.

AU - Pinard, L.

AU - Poggiani, R.

AU - Popolizio, P.

AU - Prato, M.

AU - Puppo, P.

AU - Rabeling, D.

AU - Rapagnani, P.

AU - Read, J.

AU - Regimbau, T.

AU - Rehbein, H.

AU - Reid, S.

AU - Rezzolla, L.

AU - Ricci, F.

AU - Richard, F.

AU - Rocchi, A.

AU - Rowan, S.

AU - Rüdiger, A.

AU - Sassolas, B.

AU - Sathyaprakash, B.

AU - Schnabel, R.

AU - Schwarz, C.

AU - Seidel, P.

AU - Sintes, A.

AU - Somiya, K.

AU - Speirits, F.

AU - Strain, K.

AU - Strigin, S.

AU - Sutton, P.

AU - Tarabrin, S.

AU - Van Den Brand, J.

AU - Van Leewen, C.

AU - Van Veggel, M.

AU - Van Den Broeck, C.

AU - Vecchio, A.

AU - Veitch, J.

AU - Vetrano, F.

AU - Vicere, A.

AU - Vyatchanin, S.

AU - Willke, B.

AU - Woan, G.

AU - Wolfango, P.

AU - Yamamoto, K.

PY - 2010

Y1 - 2010

N2 - Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported.

AB - Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported.

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UR - http://www.scopus.com/inward/citedby.url?scp=77950586634&partnerID=8YFLogxK

U2 - 10.1088/0264-9381/27/8/084007

DO - 10.1088/0264-9381/27/8/084007

M3 - Article

AN - SCOPUS:77950586634

SN - 0264-9381

VL - 27

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 8

M1 - 084007

ER -

The third generation of gravitational wave observatories and their science reach

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