Sensitivity studies for third-generation gravitational wave observatories

S. Hild; M. Abernathy; F. Acernese; P. Amaro-Seoane; 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; 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; D. Friedrich; P. Fulda; J. Gair; G. Gemme; E. Genin; A. Gennai; A. Giazotto; K. Glampedakis; C. Gräf; M. Granata; H. Grote; G. Guidi; A. Gurkovsky; G. Hammond; M. Hannam; J. Harms; D. Heinert; M. Hendry; I. Heng; E. Hennes; J. Hough; S. Husa; S. Huttner; G. Jones; F. Khalili; K. Kokeyama; K. Kokkotas; B. Krishnan; T.G.F. Li; M. Lorenzini; H. Lück; E. Majorana; I. Mandel; V. Mandic; M. Mantovani; I. Martin; C. Michel; Y. Minenkov; N. Morgado; S. Mosca; B. Mours; H. MüllerEbhardt; 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; W. Plastino; R. Poggiani; P. Popolizio; M. Prato; M. Punturo; P. Puppo; D. Rabeling; P. Rapagnani; J. Read; T. Regimbau; H. Rehbein; S. Reid; F. Ricci; F. Richard; A. Rocchi; S. Rowan; A. Rüdiger; L. Santamaría; B. Sassolas; B. Sathyaprakash; R. Schnabel; C. Schwarz; P. Seidel; A. Sintes; K. Somiya; F. Speirits; K. Strain; S. Strigin; P. Sutton; S. Tarabrin; A. Thüring; J. Van Den Brand; M. Van Veggel; C. Van Den Broeck; A. Vecchio; J. Veitch; F. Vetrano; A. Vicere; S. Vyatchanin; B. Willke; G. Woan; K. Yamamoto

doi:10.1088/0264-9381/28/9/094013

Sensitivity studies for third-generation gravitational wave observatories

S. Hild, M. Abernathy, F. Acernese, P. Amaro-Seoane, 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, 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, D. Friedrich, P. Fulda, J. Gair, G. Gemme, E. Genin, A. Gennai, A. Giazotto, K. Glampedakis, C. Gräf, M. Granata, H. Grote, G. Guidi, A. Gurkovsky, G. Hammond, M. Hannam, J. Harms, D. Heinert, M. Hendry, I. Heng, E. Hennes, J. Hough, S. Husa, S. Huttner, G. Jones, F. Khalili, K. Kokeyama, K. Kokkotas, B. Krishnan, T.G.F. Li, M. Lorenzini, H. Lück, E. Majorana, I. Mandel, V. Mandic, M. Mantovani, I. Martin, C. Michel, Y. Minenkov, N. Morgado, S. Mosca, B. Mours, H. MüllerEbhardt, 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, W. Plastino, R. Poggiani, P. Popolizio, M. Prato, M. Punturo, P. Puppo, D. Rabeling, P. Rapagnani, J. Read, T. Regimbau, H. Rehbein, S. Reid, F. Ricci, F. Richard, A. Rocchi, S. Rowan, A. Rüdiger, L. Santamaría, B. Sassolas, B. Sathyaprakash, R. Schnabel, C. Schwarz, P. Seidel, A. Sintes, K. Somiya, F. Speirits, K. Strain, S. Strigin, P. Sutton, S. Tarabrin, A. Thüring, J. Van Den Brand, M. Van Veggel, C. Van Den Broeck, A. Vecchio, J. Veitch, F. Vetrano, A. Vicere, S. Vyatchanin, B. Willke, G. Woan, K. Yamamoto

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

Abstract

Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions. © 2011 IOP Publishing Ltd.

Original language	English
Journal	Classical and Quantum Gravity
Volume	28
Issue number	9
DOIs	https://doi.org/10.1088/0264-9381/28/9/094013
Publication status	Published - 7 May 2011
Externally published	Yes

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10.1088/0264-9381/28/9/094013

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Hild, S., Abernathy, M., Acernese, F., Amaro-Seoane, P., 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. (2011). Sensitivity studies for third-generation gravitational wave observatories. Classical and Quantum Gravity, 28(9). https://doi.org/10.1088/0264-9381/28/9/094013

@article{6e386fa792ae4036bae01ad9fc88a5e7,

title = "Sensitivity studies for third-generation gravitational wave observatories",

abstract = "Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions. {\textcopyright} 2011 IOP Publishing Ltd.",

author = "S. Hild and M. Abernathy and F. Acernese and P. Amaro-Seoane 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 {Chassande Mottin}, E. 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 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 D. Friedrich and P. Fulda and J. Gair and G. Gemme and E. Genin and A. Gennai and A. Giazotto and K. Glampedakis and C. Gr{\"a}f and M. Granata and H. Grote and G. Guidi and A. Gurkovsky and G. Hammond and M. Hannam and J. Harms and D. Heinert and M. Hendry and I. Heng and E. Hennes and J. Hough and S. Husa and S. Huttner and G. Jones and F. Khalili and K. Kokeyama and K. Kokkotas and B. Krishnan and T.G.F. Li and M. Lorenzini and H. L{\"u}ck and E. Majorana and I. Mandel and V. Mandic and M. Mantovani and I. Martin and C. Michel and Y. Minenkov and N. Morgado and S. Mosca and B. Mours and H. M{\"u}llerEbhardt and P. Murray and R. Nawrodt and J. Nelson and R. Oshaughnessy and C.D. Ott and C. Palomba and A. Paoli and G. Parguez and A. Pasqualetti and R. Passaquieti and D. Passuello and L. Pinard and W. Plastino and R. Poggiani and P. Popolizio and M. Prato and M. Punturo and P. Puppo and D. Rabeling and P. Rapagnani and J. Read and T. Regimbau and H. Rehbein and S. Reid and F. Ricci and F. Richard and A. Rocchi and S. Rowan and A. R{\"u}diger and L. Santamar{\'i}a and B. Sassolas and B. Sathyaprakash and R. Schnabel and C. Schwarz and P. Seidel and A. Sintes and K. Somiya and F. Speirits and K. Strain and S. Strigin and P. Sutton and S. Tarabrin and A. Th{\"u}ring and {Van Den Brand}, J. and {Van Veggel}, M. and {Van Den Broeck}, C. and A. Vecchio and J. Veitch and F. Vetrano and A. Vicere and S. Vyatchanin and B. Willke and G. Woan and K. Yamamoto",

year = "2011",

month = may,

day = "7",

doi = "10.1088/0264-9381/28/9/094013",

language = "English",

volume = "28",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "9",

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Hild, S, Abernathy, M, Acernese, F, Amaro-Seoane, P, 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 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, Friedrich, D, Fulda, P, Gair, J, Gemme, G, Genin, E, Gennai, A, Giazotto, A, Glampedakis, K, Gräf, C, Granata, M, Grote, H, Guidi, G, Gurkovsky, A, Hammond, G, Hannam, M, Harms, J, Heinert, D, Hendry, M, Heng, I, Hennes, E, Hough, J, Husa, S, Huttner, S, Jones, G, Khalili, F, Kokeyama, K, Kokkotas, K, Krishnan, B, Li, TGF, Lorenzini, M, Lück, H, Majorana, E, Mandel, I, Mandic, V, Mantovani, M, Martin, I, Michel, C, Minenkov, Y, Morgado, N, Mosca, S, Mours, B, MüllerEbhardt, 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, Plastino, W, Poggiani, R, Popolizio, P, Prato, M, Punturo, M, Puppo, P, Rabeling, D, Rapagnani, P, Read, J, Regimbau, T, Rehbein, H, Reid, S, Ricci, F, Richard, F, Rocchi, A, Rowan, S, Rüdiger, A, Santamaría, L, Sassolas, B, Sathyaprakash, B, Schnabel, R, Schwarz, C, Seidel, P, Sintes, A, Somiya, K, Speirits, F, Strain, K, Strigin, S, Sutton, P, Tarabrin, S, Thüring, A, Van Den Brand, J, Van Veggel, M, Van Den Broeck, C, Vecchio, A, Veitch, J, Vetrano, F, Vicere, A, Vyatchanin, S, Willke, B, Woan, G & Yamamoto, K 2011, 'Sensitivity studies for third-generation gravitational wave observatories', Classical and Quantum Gravity, vol. 28, no. 9. https://doi.org/10.1088/0264-9381/28/9/094013

TY - JOUR

T1 - Sensitivity studies for third-generation gravitational wave observatories

AU - Hild, S.

AU - Abernathy, M.

AU - Acernese, F.

AU - Amaro-Seoane, P.

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 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 - Friedrich, D.

AU - Fulda, P.

AU - Gair, J.

AU - Gemme, G.

AU - Genin, E.

AU - Gennai, A.

AU - Giazotto, A.

AU - Glampedakis, K.

AU - Gräf, C.

AU - Granata, M.

AU - Grote, H.

AU - Guidi, G.

AU - Gurkovsky, A.

AU - Hammond, G.

AU - Hannam, M.

AU - Harms, J.

AU - Heinert, D.

AU - Hendry, M.

AU - Heng, I.

AU - Hennes, E.

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 - Li, T.G.F.

AU - Lorenzini, M.

AU - Lück, H.

AU - Majorana, E.

AU - Mandel, I.

AU - Mandic, V.

AU - Mantovani, M.

AU - Martin, I.

AU - Michel, C.

AU - Minenkov, Y.

AU - Morgado, N.

AU - Mosca, S.

AU - Mours, B.

AU - MüllerEbhardt, 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 - Plastino, W.

AU - Poggiani, R.

AU - Popolizio, P.

AU - Prato, M.

AU - Punturo, M.

AU - Puppo, P.

AU - Rabeling, D.

AU - Rapagnani, P.

AU - Read, J.

AU - Regimbau, T.

AU - Rehbein, H.

AU - Reid, S.

AU - Ricci, F.

AU - Richard, F.

AU - Rocchi, A.

AU - Rowan, S.

AU - Rüdiger, A.

AU - Santamaría, L.

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 - Thüring, A.

AU - Van Den Brand, J.

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 - Yamamoto, K.

PY - 2011/5/7

Y1 - 2011/5/7

N2 - Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions. © 2011 IOP Publishing Ltd.

AB - Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions. © 2011 IOP Publishing Ltd.

U2 - 10.1088/0264-9381/28/9/094013

DO - 10.1088/0264-9381/28/9/094013

M3 - Article

SN - 0264-9381

VL - 28

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 9

ER -

Sensitivity studies for third-generation gravitational wave observatories

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