The Virgo interferometric gravitational antenna

F. Acernese; P. Amico; M. Al-Shourbagy; S. Aoudia; S. Avino; D. Babusci; G. Ballardin; R. Barillé; F. Barone; L. Barsotti; M. Barsuglia; F. Beauville; M.A. Bizouard; C. Boccara; F. Bondu; L. Bosi; C. Bradaschia; S. Braccini; A. Brillet; V. Brisson; L. Brocco; D. Buskulic; E. Calloni; E. Campagna; F. Cavalier; R. Cavalieri; G. Cella; E. Chassande-Mottin; A.C. Clapson; F. Cleva; C. Corda; J.-P. Coulon; E. Cuoco; V. Dattilo; M. Davier; R. De Rosa; L. Di Fiore; A. Di Virgilio; B. Dujardin; A. Eleuteri; D. Enard; I. Ferrante; F. Fidecaro; I. Fiori; R. Flaminio; J.-D. Fournier; S. Frasca; F. Frasconi; A. Freise; L. Gammaitoni; A. Gennai; A. Giazotto; G. Giordano; R. Gouaty; D. Grosjean; G. Guidi; S. Hebri; H. Heitmann; P. Hello; L. Holloway; S. Kreckelberg; P. La Penna; V. Loriette; M. Loupias; G. Losurdo; J.-M. Mackowski; E. Majorana; C.N. Man; M. Mantovani; F. Marion; J. Marque; F. Martelli; A. Masserot; L. Massonnet; M. Mazzoni; L. Milano; C. Moins; J. Moreau; F. Moreau; N. Morgado; F. Mornet; B. Mours; J. Pacheco; A. Pai; C. Palomba; F. Paoletti; S. Pardi; A. Pasqualetti; R. Passaquieti; D. Passuello; B. Perniola; F. Piergiovanni; L. Pinard; R. Poggiani; M. Punturo; P. Puppo; K. Qipiani; P. Rapagnani; V. Reita; A. Remillieux; F. Ricci; I. Ricciardi; P. Ruggi; G. Russo; S. Solimeno; A. Spallicci; R. Stanga; R. Taddei; D. Tombolato; A. Toncelli; M. Tonelli; E. Tournefier; F. Travasso; H. Trinquet; M. Varvella; D. Verkindt; F. Vetrano; A. Viceré; J.-Y. Vinet; H. Vocca; M. Yvert; Z. Zhou

doi:10.1016/j.optlaseng.2006.04.010

The Virgo interferometric gravitational antenna

F. Acernese, P. Amico, M. Al-Shourbagy, S. Aoudia, S. Avino, D. Babusci, G. Ballardin, R. Barillé, F. Barone, L. Barsotti, M. Barsuglia, F. Beauville, M.A. Bizouard, C. Boccara, F. Bondu, L. Bosi, C. Bradaschia, S. Braccini, A. Brillet, V. BrissonL. Brocco, D. Buskulic, E. Calloni, E. Campagna, F. Cavalier, R. Cavalieri, G. Cella, E. Chassande-Mottin, A.C. Clapson, F. Cleva, C. Corda, J.-P. Coulon, E. Cuoco, V. Dattilo, M. Davier, R. De Rosa, L. Di Fiore, A. Di Virgilio, B. Dujardin, A. Eleuteri, D. Enard, I. Ferrante, F. Fidecaro, I. Fiori, R. Flaminio, J.-D. Fournier, S. Frasca, F. Frasconi, A. Freise, L. Gammaitoni, A. Gennai, A. Giazotto, G. Giordano, R. Gouaty, D. Grosjean, G. Guidi, S. Hebri, H. Heitmann, P. Hello, L. Holloway, S. Kreckelberg, P. La Penna, V. Loriette, M. Loupias, G. Losurdo, J.-M. Mackowski, E. Majorana, C.N. Man, M. Mantovani, F. Marion, J. Marque, F. Martelli, A. Masserot, L. Massonnet, M. Mazzoni, L. Milano, C. Moins, J. Moreau, F. Moreau, N. Morgado, F. Mornet, B. Mours, J. Pacheco, A. Pai, C. Palomba, F. Paoletti, S. Pardi, A. Pasqualetti, R. Passaquieti, D. Passuello, B. Perniola, F. Piergiovanni, L. Pinard, R. Poggiani, M. Punturo, P. Puppo, K. Qipiani, P. Rapagnani, V. Reita, A. Remillieux, F. Ricci, I. Ricciardi, P. Ruggi, G. Russo, S. Solimeno, A. Spallicci, R. Stanga, R. Taddei, D. Tombolato, A. Toncelli, M. Tonelli, E. Tournefier, F. Travasso, H. Trinquet, M. Varvella, D. Verkindt, F. Vetrano, A. Viceré, J.-Y. Vinet, H. Vocca, M. Yvert, Z. Zhou

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

Abstract

The interferometric gravitational wave detectors represent the ultimate evolution of the classical Michelson interferometer. In order to measure the signal produced by the passage of a gravitational wave, they aim to reach unprecedent sensitivities in measuring the relative displacements of the mirrors. One of them, the 3-km-long Virgo gravitational wave antenna, which will be particularly sensitive in the low-frequency range (10-100 Hz), is presently in its commissioning phase. In this paper the various techniques developed in order to reach its target extreme performance are outlined. © 2006 Elsevier Ltd. All rights reserved.

Original language	English
Pages (from-to)	478-487
Journal	Optics and Lasers in Engineering
Volume	45
Issue number	4
DOIs	https://doi.org/10.1016/j.optlaseng.2006.04.010
Publication status	Published - 2007
Externally published	Yes

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Acernese, F., Amico, P., Al-Shourbagy, M., Aoudia, S., Avino, S., Babusci, D., Ballardin, G., Barillé, R., Barone, F., Barsotti, L., Barsuglia, M., Beauville, F., Bizouard, M. A., Boccara, C., Bondu, F., Bosi, L., Bradaschia, C., Braccini, S., Brillet, A., ... Zhou, Z. (2007). The Virgo interferometric gravitational antenna. Optics and Lasers in Engineering, 45(4), 478-487. https://doi.org/10.1016/j.optlaseng.2006.04.010

@article{54f4920180bc45088039fd5da27f19c3,

title = "The Virgo interferometric gravitational antenna",

abstract = "The interferometric gravitational wave detectors represent the ultimate evolution of the classical Michelson interferometer. In order to measure the signal produced by the passage of a gravitational wave, they aim to reach unprecedent sensitivities in measuring the relative displacements of the mirrors. One of them, the 3-km-long Virgo gravitational wave antenna, which will be particularly sensitive in the low-frequency range (10-100 Hz), is presently in its commissioning phase. In this paper the various techniques developed in order to reach its target extreme performance are outlined. {\textcopyright} 2006 Elsevier Ltd. All rights reserved.",

author = "F. Acernese and P. Amico and M. Al-Shourbagy and S. Aoudia and S. Avino and D. Babusci and G. Ballardin and R. Barill{\'e} and F. Barone and L. Barsotti and M. Barsuglia and F. Beauville and M.A. Bizouard and C. Boccara and F. Bondu and L. Bosi and C. Bradaschia and S. Braccini and A. Brillet and V. Brisson and L. Brocco and D. Buskulic and E. Calloni and E. Campagna and F. Cavalier and R. Cavalieri and G. Cella and E. Chassande-Mottin and A.C. Clapson and F. Cleva and C. Corda and J.-P. Coulon and E. Cuoco and V. Dattilo and M. Davier and {De Rosa}, R. and {Di Fiore}, L. and {Di Virgilio}, A. and B. Dujardin and A. Eleuteri and D. Enard and I. Ferrante and F. Fidecaro and I. Fiori and R. Flaminio and J.-D. Fournier and S. Frasca and F. Frasconi and A. Freise and L. Gammaitoni and A. Gennai and A. Giazotto and G. Giordano and R. Gouaty and D. Grosjean and G. Guidi and S. Hebri and H. Heitmann and P. Hello and L. Holloway and S. Kreckelberg and {La Penna}, P. and V. Loriette and M. Loupias and G. Losurdo and J.-M. Mackowski and E. Majorana and C.N. Man and M. Mantovani and F. Marion and J. Marque and F. Martelli and A. Masserot and L. Massonnet and M. Mazzoni and L. Milano and C. Moins and J. Moreau and F. Moreau and N. Morgado and F. Mornet and B. Mours and J. Pacheco and A. Pai and C. Palomba and F. Paoletti and S. Pardi and A. Pasqualetti and R. Passaquieti and D. Passuello and B. Perniola and F. Piergiovanni and L. Pinard and R. Poggiani and M. Punturo and P. Puppo and K. Qipiani and P. Rapagnani and V. Reita and A. Remillieux and F. Ricci and I. Ricciardi and P. Ruggi and G. Russo and S. Solimeno and A. Spallicci and R. Stanga and R. Taddei and D. Tombolato and A. Toncelli and M. Tonelli and E. Tournefier and F. Travasso and H. Trinquet and M. Varvella and D. Verkindt and F. Vetrano and A. Vicer{\'e} and J.-Y. Vinet and H. Vocca and M. Yvert and Z. Zhou",

year = "2007",

doi = "10.1016/j.optlaseng.2006.04.010",

language = "English",

volume = "45",

pages = "478--487",

journal = "Optics and Lasers in Engineering",

issn = "0143-8166",

publisher = "Elsevier Ltd",

number = "4",

}

Acernese, F, Amico, P, Al-Shourbagy, M, Aoudia, S, Avino, S, Babusci, D, Ballardin, G, Barillé, R, Barone, F, Barsotti, L, Barsuglia, M, Beauville, F, Bizouard, MA, Boccara, C, Bondu, F, Bosi, L, Bradaschia, C, Braccini, S, Brillet, A, Brisson, V, Brocco, L, Buskulic, D, Calloni, E, Campagna, E, Cavalier, F, Cavalieri, R, Cella, G, Chassande-Mottin, E, Clapson, AC, Cleva, F, Corda, C, Coulon, J-P, Cuoco, E, Dattilo, V, Davier, M, De Rosa, R, Di Fiore, L, Di Virgilio, A, Dujardin, B, Eleuteri, A, Enard, D, Ferrante, I, Fidecaro, F, Fiori, I, Flaminio, R, Fournier, J-D, Frasca, S, Frasconi, F, Freise, A, Gammaitoni, L, Gennai, A, Giazotto, A, Giordano, G, Gouaty, R, Grosjean, D, Guidi, G, Hebri, S, Heitmann, H, Hello, P, Holloway, L, Kreckelberg, S, La Penna, P, Loriette, V, Loupias, M, Losurdo, G, Mackowski, J-M, Majorana, E, Man, CN, Mantovani, M, Marion, F, Marque, J, Martelli, F, Masserot, A, Massonnet, L, Mazzoni, M, Milano, L, Moins, C, Moreau, J, Moreau, F, Morgado, N, Mornet, F, Mours, B, Pacheco, J, Pai, A, Palomba, C, Paoletti, F, Pardi, S, Pasqualetti, A, Passaquieti, R, Passuello, D, Perniola, B, Piergiovanni, F, Pinard, L, Poggiani, R, Punturo, M, Puppo, P, Qipiani, K, Rapagnani, P, Reita, V, Remillieux, A, Ricci, F, Ricciardi, I, Ruggi, P, Russo, G, Solimeno, S, Spallicci, A, Stanga, R, Taddei, R, Tombolato, D, Toncelli, A, Tonelli, M, Tournefier, E, Travasso, F, Trinquet, H, Varvella, M, Verkindt, D, Vetrano, F, Viceré, A, Vinet, J-Y, Vocca, H, Yvert, M & Zhou, Z 2007, 'The Virgo interferometric gravitational antenna', Optics and Lasers in Engineering, vol. 45, no. 4, pp. 478-487. https://doi.org/10.1016/j.optlaseng.2006.04.010

TY - JOUR

T1 - The Virgo interferometric gravitational antenna

AU - Acernese, F.

AU - Amico, P.

AU - Al-Shourbagy, M.

AU - Aoudia, S.

AU - Avino, S.

AU - Babusci, D.

AU - Ballardin, G.

AU - Barillé, R.

AU - Barone, F.

AU - Barsotti, L.

AU - Barsuglia, M.

AU - Beauville, F.

AU - Bizouard, M.A.

AU - Boccara, C.

AU - Bondu, F.

AU - Bosi, L.

AU - Bradaschia, C.

AU - Braccini, S.

AU - Brillet, A.

AU - Brisson, V.

AU - Brocco, L.

AU - Buskulic, D.

AU - Calloni, E.

AU - Campagna, E.

AU - Cavalier, F.

AU - Cavalieri, R.

AU - Cella, G.

AU - Chassande-Mottin, E.

AU - Clapson, A.C.

AU - Cleva, F.

AU - Corda, C.

AU - Coulon, J.-P.

AU - Cuoco, E.

AU - Dattilo, V.

AU - Davier, M.

AU - De Rosa, R.

AU - Di Fiore, L.

AU - Di Virgilio, A.

AU - Dujardin, B.

AU - Eleuteri, A.

AU - Enard, D.

AU - Ferrante, I.

AU - Fidecaro, F.

AU - Fiori, I.

AU - Flaminio, R.

AU - Fournier, J.-D.

AU - Frasca, S.

AU - Frasconi, F.

AU - Freise, A.

AU - Gammaitoni, L.

AU - Gennai, A.

AU - Giazotto, A.

AU - Giordano, G.

AU - Gouaty, R.

AU - Grosjean, D.

AU - Guidi, G.

AU - Hebri, S.

AU - Heitmann, H.

AU - Hello, P.

AU - Holloway, L.

AU - Kreckelberg, S.

AU - La Penna, P.

AU - Loriette, V.

AU - Loupias, M.

AU - Losurdo, G.

AU - Mackowski, J.-M.

AU - Majorana, E.

AU - Man, C.N.

AU - Mantovani, M.

AU - Marion, F.

AU - Marque, J.

AU - Martelli, F.

AU - Masserot, A.

AU - Massonnet, L.

AU - Mazzoni, M.

AU - Milano, L.

AU - Moins, C.

AU - Moreau, J.

AU - Moreau, F.

AU - Morgado, N.

AU - Mornet, F.

AU - Mours, B.

AU - Pacheco, J.

AU - Pai, A.

AU - Palomba, C.

AU - Paoletti, F.

AU - Pardi, S.

AU - Pasqualetti, A.

AU - Passaquieti, R.

AU - Passuello, D.

AU - Perniola, B.

AU - Piergiovanni, F.

AU - Pinard, L.

AU - Poggiani, R.

AU - Punturo, M.

AU - Puppo, P.

AU - Qipiani, K.

AU - Rapagnani, P.

AU - Reita, V.

AU - Remillieux, A.

AU - Ricci, F.

AU - Ricciardi, I.

AU - Ruggi, P.

AU - Russo, G.

AU - Solimeno, S.

AU - Spallicci, A.

AU - Stanga, R.

AU - Taddei, R.

AU - Tombolato, D.

AU - Toncelli, A.

AU - Tonelli, M.

AU - Tournefier, E.

AU - Travasso, F.

AU - Trinquet, H.

AU - Varvella, M.

AU - Verkindt, D.

AU - Vetrano, F.

AU - Viceré, A.

AU - Vinet, J.-Y.

AU - Vocca, H.

AU - Yvert, M.

AU - Zhou, Z.

PY - 2007

Y1 - 2007

N2 - The interferometric gravitational wave detectors represent the ultimate evolution of the classical Michelson interferometer. In order to measure the signal produced by the passage of a gravitational wave, they aim to reach unprecedent sensitivities in measuring the relative displacements of the mirrors. One of them, the 3-km-long Virgo gravitational wave antenna, which will be particularly sensitive in the low-frequency range (10-100 Hz), is presently in its commissioning phase. In this paper the various techniques developed in order to reach its target extreme performance are outlined. © 2006 Elsevier Ltd. All rights reserved.

AB - The interferometric gravitational wave detectors represent the ultimate evolution of the classical Michelson interferometer. In order to measure the signal produced by the passage of a gravitational wave, they aim to reach unprecedent sensitivities in measuring the relative displacements of the mirrors. One of them, the 3-km-long Virgo gravitational wave antenna, which will be particularly sensitive in the low-frequency range (10-100 Hz), is presently in its commissioning phase. In this paper the various techniques developed in order to reach its target extreme performance are outlined. © 2006 Elsevier Ltd. All rights reserved.

U2 - 10.1016/j.optlaseng.2006.04.010

DO - 10.1016/j.optlaseng.2006.04.010

M3 - Article

SN - 0143-8166

VL - 45

SP - 478

EP - 487

JO - Optics and Lasers in Engineering

JF - Optics and Lasers in Engineering

IS - 4

ER -

The Virgo interferometric gravitational antenna

Abstract

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