Performances of the Virgo interferometer longitudinal control system

F. Acernese; F. Antonucci; S. Aoudia; K. G. Arun; P. Astone; G. Ballardin; F. Barone; M. Barsuglia; Th S. Bauer; M. G. Beker; S. Bigotta; S. Birindelli; M. A. Bizouard; M. Blom; C. Boccara; F. Bondu; L. Bonelli; L. Bosi; S. Braccini; C. Bradaschia; A. Brillet; V. Brisson; R. Budzyński; T. Bulik; H. J. Bulten; D. Buskulic; G. Cagnoli; E. Calloni; E. Campagna; B. Canuel; F. Carbognani; F. Cavalier; R. Cavalieri; G. Cella; E. Cesarini; E. Chassande-Mottin; A. Chincarini; F. Cleva; E. Coccia; C. N. Colacino; J. Colas; A. Colla; M. Colombini; C. Corda; A. Corsi; J. P. Coulon; E. Cuoco; S. D'Antonio; A. Dari; V. Dattilo; M. Davier; R. Day; R. De Rosa; M. del Prete; L. Di Fiore; A. Di Lieto; M. Di Paolo Emilio; A. Di Virgilio; A. Dietz; M. Drago; V. Fafone; I. Ferrante; F. Fidecaro; I. Fiori; R. Flaminio; J. D. Fournier; J. Franc; S. Frasca; F. Frasconi; A. Freise; L. Gammaitoni; F. Garufi; G. Gemme; E. Genin; A. Gennai; A. Giazotto; M. Granata; C. Greverie; G. Guidi; H. Heitmann; P. Hello; S. Hild; D. Huet; P. Jaranowski; I. Kowalska; A. Królak; P. La Penna; N. Leroy; N. Letendre; T. G.F. Li; M. Lorenzini; V. Loriette; G. Losurdo; J. M. Mackowski; E. Majorana; N. Man; M. Mantovani; F. Marchesoni; F. Marion; J. Marque; F. Martelli; A. Masserot; F. Menzinger; C. Michel; L. Milano; Y. Minenkov; M. Mohan; J. Moreau; N. Morgado; A. Morgia; S. Mosca; V. Moscatelli; B. Mours; I. Neri; F. Nocera; G. Pagliaroli; C. Palomba; F. Paoletti; S. Pardi; M. Parisi; A. Pasqualetti; R. Passaquieti; D. Passuello; G. Persichetti; M. Pichot; F. Piergiovanni; M. Pietka; L. Pinard; R. Poggiani; M. Prato; G. A. Prodi; M. Punturo; P. Puppo; O. Rabaste; D. S. Rabeling; P. Rapagnani; V. Re; T. Regimbau; F. Ricci; F. Robinet; A. Rocchi; L. Rolland; R. Romano; D. Rosińska; P. Ruggi; F. Salemi; B. Sassolas; D. Sentenac; R. Sturani; B. Swinkels; A. Toncelli; M. Tonelli; E. Tournefier; F. Travasso; J. Trummer; G. Vajente; J. F.J. van den Brand; S. van der Putten; M. Vavoulidis; G. Vedovato; D. Verkindt; F. Vetrano; A. Viceré; J. Y. Vinet; H. Vocca; M. Was; M. Yvert

doi:10.1016/j.astropartphys.2009.11.006

Performances of the Virgo interferometer longitudinal control system

F. Acernese, F. Antonucci, S. Aoudia, K. G. Arun, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, Th S. Bauer, M. G. Beker, S. Bigotta, S. Birindelli, M. A. Bizouard, M. Blom, C. Boccara, F. Bondu, L. Bonelli, L. Bosi, S. Braccini, C. BradaschiaA. Brillet, V. Brisson, R. Budzyński, T. Bulik, H. J. Bulten, D. Buskulic, G. Cagnoli, E. Calloni, E. Campagna, B. Canuel, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, E. Chassande-Mottin, A. Chincarini, F. Cleva, E. Coccia, C. N. Colacino, J. Colas, A. Colla, M. Colombini, C. Corda, A. Corsi, J. P. Coulon, E. Cuoco, S. D'Antonio, A. Dari, V. Dattilo, M. Davier, R. Day, R. De Rosa, M. del Prete, L. Di Fiore, A. Di Lieto, M. Di Paolo Emilio, A. Di Virgilio, A. Dietz, M. Drago, V. Fafone, I. Ferrante, F. Fidecaro, I. Fiori, R. Flaminio, J. D. Fournier, J. Franc, S. Frasca, F. Frasconi, A. Freise, L. Gammaitoni, F. Garufi, G. Gemme, E. Genin, A. Gennai, A. Giazotto, M. Granata, C. Greverie, G. Guidi, H. Heitmann, P. Hello, S. Hild, D. Huet, P. Jaranowski, I. Kowalska, A. Królak, P. La Penna, N. Leroy, N. Letendre, T. G.F. Li, M. Lorenzini, V. Loriette, G. Losurdo, J. M. Mackowski, E. Majorana, N. Man, M. Mantovani, F. Marchesoni, F. Marion, J. Marque, F. Martelli, A. Masserot, F. Menzinger, C. Michel, L. Milano, Y. Minenkov, M. Mohan, J. Moreau, N. Morgado, A. Morgia, S. Mosca, V. Moscatelli, B. Mours, I. Neri, F. Nocera, G. Pagliaroli, C. Palomba, F. Paoletti, S. Pardi, M. Parisi, A. Pasqualetti, R. Passaquieti, D. Passuello, G. Persichetti, M. Pichot, F. Piergiovanni, M. Pietka, L. Pinard, R. Poggiani, M. Prato, G. A. Prodi, M. Punturo, P. Puppo, O. Rabaste, D. S. Rabeling, P. Rapagnani, V. Re, T. Regimbau, F. Ricci, F. Robinet, A. Rocchi, L. Rolland, R. Romano, D. Rosińska, P. Ruggi, F. Salemi, B. Sassolas, D. Sentenac, R. Sturani, B. Swinkels, A. Toncelli, M. Tonelli, E. Tournefier, F. Travasso, J. Trummer, G. Vajente, J. F.J. van den Brand, S. van der Putten, M. Vavoulidis, G. Vedovato, D. Verkindt, F. Vetrano, A. Viceré, J. Y. Vinet, H. Vocca, M. Was, M. Yvert

Physics

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

11 Scopus citations

Abstract

The performances of the longitudinal sensing and control system of the Virgo gravitational wave detector are described. This system is able to stably maintain the RMS residual fluctuation of the interferometer longitudinal degrees of freedom around or below 10^{- 11} m, compatible with the original Virgo requirements. Moreover the detector sensitivity is not limited by longitudinal control noise at any frequency. Indeed the noise re-introduced by the longitudinal control system does not affect the Virgo design sensitivity.

Original language	English
Pages (from-to)	75-80
Number of pages	6
Journal	Astroparticle Physics
Volume	33
Issue number	2
DOIs	https://doi.org/10.1016/j.astropartphys.2009.11.006
State	Published - Mar 2010

Keywords

Gravitational waves
Interferometry
Virgo

Access to Document

10.1016/j.astropartphys.2009.11.006

Cite this

Acernese, F., Antonucci, F., Aoudia, S., Arun, K. G., Astone, P., Ballardin, G., Barone, F., Barsuglia, M., Bauer, T. S., Beker, M. G., Bigotta, S., Birindelli, S., Bizouard, M. A., Blom, M., Boccara, C., Bondu, F., Bonelli, L., Bosi, L., Braccini, S., ... Yvert, M. (2010). Performances of the Virgo interferometer longitudinal control system. Astroparticle Physics, 33(2), 75-80. https://doi.org/10.1016/j.astropartphys.2009.11.006

@article{de97a61095484255ae8905a146bd7784,

title = "Performances of the Virgo interferometer longitudinal control system",

abstract = "The performances of the longitudinal sensing and control system of the Virgo gravitational wave detector are described. This system is able to stably maintain the RMS residual fluctuation of the interferometer longitudinal degrees of freedom around or below 10- 11 m, compatible with the original Virgo requirements. Moreover the detector sensitivity is not limited by longitudinal control noise at any frequency. Indeed the noise re-introduced by the longitudinal control system does not affect the Virgo design sensitivity.",

keywords = "Gravitational waves, Interferometry, Virgo",

author = "F. Acernese and F. Antonucci and S. Aoudia and Arun, {K. G.} and P. Astone and G. Ballardin and F. Barone and M. Barsuglia and Bauer, {Th S.} and Beker, {M. G.} and S. Bigotta and S. Birindelli and Bizouard, {M. A.} and M. Blom and C. Boccara and F. Bondu and L. Bonelli and L. Bosi and S. Braccini and C. Bradaschia and A. Brillet and V. Brisson and R. Budzy{\'n}ski and T. Bulik and Bulten, {H. J.} and D. Buskulic and G. Cagnoli and E. Calloni and E. Campagna and B. Canuel and F. Carbognani and F. Cavalier and R. Cavalieri and G. Cella and E. Cesarini and E. Chassande-Mottin and A. Chincarini and F. Cleva and E. Coccia and Colacino, {C. N.} and J. Colas and A. Colla and M. Colombini and C. Corda and A. Corsi and Coulon, {J. P.} and E. Cuoco and S. D'Antonio and A. Dari and V. Dattilo and M. Davier and R. Day and {De Rosa}, R. and {del Prete}, M. and {Di Fiore}, L. and {Di Lieto}, A. and {Di Paolo Emilio}, M. and {Di Virgilio}, A. and A. Dietz and M. Drago and V. Fafone and I. Ferrante and F. Fidecaro and I. Fiori and R. Flaminio and Fournier, {J. D.} and J. Franc and S. Frasca and F. Frasconi and A. Freise and L. Gammaitoni and F. Garufi and G. Gemme and E. Genin and A. Gennai and A. Giazotto and M. Granata and C. Greverie and G. Guidi and H. Heitmann and P. Hello and S. Hild and D. Huet and P. Jaranowski and I. Kowalska and A. Kr{\'o}lak and {La Penna}, P. and N. Leroy and N. Letendre and Li, {T. G.F.} and M. Lorenzini and V. Loriette and G. Losurdo and Mackowski, {J. M.} and E. Majorana and N. Man and M. Mantovani and F. Marchesoni and F. Marion and J. Marque and F. Martelli and A. Masserot and F. Menzinger and C. Michel and L. Milano and Y. Minenkov and M. Mohan and J. Moreau and N. Morgado and A. Morgia and S. Mosca and V. Moscatelli and B. Mours and I. Neri and F. Nocera and G. Pagliaroli and C. Palomba and F. Paoletti and S. Pardi and M. Parisi and A. Pasqualetti and R. Passaquieti and D. Passuello and G. Persichetti and M. Pichot and F. Piergiovanni and M. Pietka and L. Pinard and R. Poggiani and M. Prato and Prodi, {G. A.} and M. Punturo and P. Puppo and O. Rabaste and Rabeling, {D. S.} and P. Rapagnani and V. Re and T. Regimbau and F. Ricci and F. Robinet and A. Rocchi and L. Rolland and R. Romano and D. Rosi{\'n}ska and P. Ruggi and F. Salemi and B. Sassolas and D. Sentenac and R. Sturani and B. Swinkels and A. Toncelli and M. Tonelli and E. Tournefier and F. Travasso and J. Trummer and G. Vajente and {van den Brand}, {J. F.J.} and {van der Putten}, S. and M. Vavoulidis and G. Vedovato and D. Verkindt and F. Vetrano and A. Vicer{\'e} and Vinet, {J. Y.} and H. Vocca and M. Was and M. Yvert",

note = "Funding Information: The authors gratefully acknowledge the support of the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by the Foundation for Fundamental Research on Matter of the Netherlands Organisation for Scientific Research , the Polish Ministry of Science and Higher Education grant N N203 387237 , the FOCUS Programme of Foundation for Polish Science and the European Associated Laboratory Astrophysics Poland-France. ",

year = "2010",

month = mar,

doi = "10.1016/j.astropartphys.2009.11.006",

language = "English",

volume = "33",

pages = "75--80",

journal = "Astroparticle Physics",

issn = "0927-6505",

number = "2",

}

Acernese, F, Antonucci, F, Aoudia, S, Arun, KG, Astone, P, Ballardin, G, Barone, F, Barsuglia, M, Bauer, TS, Beker, MG, Bigotta, S, Birindelli, S, Bizouard, MA, Blom, M, Boccara, C, Bondu, F, Bonelli, L, Bosi, L, Braccini, S, Bradaschia, C, Brillet, A, Brisson, V, Budzyński, R, Bulik, T, Bulten, HJ, Buskulic, D, Cagnoli, G, Calloni, E, Campagna, E, Canuel, B, Carbognani, F, Cavalier, F, Cavalieri, R, Cella, G, Cesarini, E, Chassande-Mottin, E, Chincarini, A, Cleva, F, Coccia, E, Colacino, CN, Colas, J, Colla, A, Colombini, M, Corda, C, Corsi, A, Coulon, JP, Cuoco, E, D'Antonio, S, Dari, A, Dattilo, V, Davier, M, Day, R, De Rosa, R, del Prete, M, Di Fiore, L, Di Lieto, A, Di Paolo Emilio, M, Di Virgilio, A, Dietz, A, Drago, M, Fafone, V, Ferrante, I, Fidecaro, F, Fiori, I, Flaminio, R, Fournier, JD, Franc, J, Frasca, S, Frasconi, F, Freise, A, Gammaitoni, L, Garufi, F, Gemme, G, Genin, E, Gennai, A, Giazotto, A, Granata, M, Greverie, C, Guidi, G, Heitmann, H, Hello, P, Hild, S, Huet, D, Jaranowski, P, Kowalska, I, Królak, A, La Penna, P, Leroy, N, Letendre, N, Li, TGF, Lorenzini, M, Loriette, V, Losurdo, G, Mackowski, JM, Majorana, E, Man, N, Mantovani, M, Marchesoni, F, Marion, F, Marque, J, Martelli, F, Masserot, A, Menzinger, F, Michel, C, Milano, L, Minenkov, Y, Mohan, M, Moreau, J, Morgado, N, Morgia, A, Mosca, S, Moscatelli, V, Mours, B, Neri, I, Nocera, F, Pagliaroli, G, Palomba, C, Paoletti, F, Pardi, S, Parisi, M, Pasqualetti, A, Passaquieti, R, Passuello, D, Persichetti, G, Pichot, M, Piergiovanni, F, Pietka, M, Pinard, L, Poggiani, R, Prato, M, Prodi, GA, Punturo, M, Puppo, P, Rabaste, O, Rabeling, DS, Rapagnani, P, Re, V, Regimbau, T, Ricci, F, Robinet, F, Rocchi, A, Rolland, L, Romano, R, Rosińska, D, Ruggi, P, Salemi, F, Sassolas, B, Sentenac, D, Sturani, R, Swinkels, B, Toncelli, A, Tonelli, M, Tournefier, E, Travasso, F, Trummer, J, Vajente, G, van den Brand, JFJ, van der Putten, S, Vavoulidis, M, Vedovato, G, Verkindt, D, Vetrano, F, Viceré, A, Vinet, JY, Vocca, H, Was, M & Yvert, M 2010, 'Performances of the Virgo interferometer longitudinal control system', Astroparticle Physics, vol. 33, no. 2, pp. 75-80. https://doi.org/10.1016/j.astropartphys.2009.11.006

TY - JOUR

T1 - Performances of the Virgo interferometer longitudinal control system

AU - Acernese, F.

AU - Antonucci, F.

AU - Aoudia, S.

AU - Arun, K. G.

AU - Astone, P.

AU - Ballardin, G.

AU - Barone, F.

AU - Barsuglia, M.

AU - Bauer, Th S.

AU - Beker, M. G.

AU - Bigotta, S.

AU - Birindelli, S.

AU - Bizouard, M. A.

AU - Blom, M.

AU - Boccara, C.

AU - Bondu, F.

AU - Bonelli, L.

AU - Bosi, L.

AU - Braccini, S.

AU - Bradaschia, C.

AU - Brillet, A.

AU - Brisson, V.

AU - Budzyński, R.

AU - Bulik, T.

AU - Bulten, H. J.

AU - Buskulic, D.

AU - Cagnoli, G.

AU - Calloni, E.

AU - Campagna, E.

AU - Canuel, B.

AU - Carbognani, F.

AU - Cavalier, F.

AU - Cavalieri, R.

AU - Cella, G.

AU - Cesarini, E.

AU - Chassande-Mottin, E.

AU - Chincarini, A.

AU - Cleva, F.

AU - Coccia, E.

AU - Colacino, C. N.

AU - Colas, J.

AU - Colla, A.

AU - Colombini, M.

AU - Corda, C.

AU - Corsi, A.

AU - Coulon, J. P.

AU - Cuoco, E.

AU - D'Antonio, S.

AU - Dari, A.

AU - Dattilo, V.

AU - Davier, M.

AU - Day, R.

AU - De Rosa, R.

AU - del Prete, M.

AU - Di Fiore, L.

AU - Di Lieto, A.

AU - Di Paolo Emilio, M.

AU - Di Virgilio, A.

AU - Dietz, A.

AU - Drago, M.

AU - Fafone, V.

AU - Ferrante, I.

AU - Fidecaro, F.

AU - Fiori, I.

AU - Flaminio, R.

AU - Fournier, J. D.

AU - Franc, J.

AU - Frasca, S.

AU - Frasconi, F.

AU - Freise, A.

AU - Gammaitoni, L.

AU - Garufi, F.

AU - Gemme, G.

AU - Genin, E.

AU - Gennai, A.

AU - Giazotto, A.

AU - Granata, M.

AU - Greverie, C.

AU - Guidi, G.

AU - Heitmann, H.

AU - Hello, P.

AU - Hild, S.

AU - Huet, D.

AU - Jaranowski, P.

AU - Kowalska, I.

AU - Królak, A.

AU - La Penna, P.

AU - Leroy, N.

AU - Letendre, N.

AU - Li, T. G.F.

AU - Lorenzini, M.

AU - Loriette, V.

AU - Losurdo, G.

AU - Mackowski, J. M.

AU - Majorana, E.

AU - Man, N.

AU - Mantovani, M.

AU - Marchesoni, F.

AU - Marion, F.

AU - Marque, J.

AU - Martelli, F.

AU - Masserot, A.

AU - Menzinger, F.

AU - Michel, C.

AU - Milano, L.

AU - Minenkov, Y.

AU - Mohan, M.

AU - Moreau, J.

AU - Morgado, N.

AU - Morgia, A.

AU - Mosca, S.

AU - Moscatelli, V.

AU - Mours, B.

AU - Neri, I.

AU - Nocera, F.

AU - Pagliaroli, G.

AU - Palomba, C.

AU - Paoletti, F.

AU - Pardi, S.

AU - Parisi, M.

AU - Pasqualetti, A.

AU - Passaquieti, R.

AU - Passuello, D.

AU - Persichetti, G.

AU - Pichot, M.

AU - Piergiovanni, F.

AU - Pietka, M.

AU - Pinard, L.

AU - Poggiani, R.

AU - Prato, M.

AU - Prodi, G. A.

AU - Punturo, M.

AU - Puppo, P.

AU - Rabaste, O.

AU - Rabeling, D. S.

AU - Rapagnani, P.

AU - Re, V.

AU - Regimbau, T.

AU - Ricci, F.

AU - Robinet, F.

AU - Rocchi, A.

AU - Rolland, L.

AU - Romano, R.

AU - Rosińska, D.

AU - Ruggi, P.

AU - Salemi, F.

AU - Sassolas, B.

AU - Sentenac, D.

AU - Sturani, R.

AU - Swinkels, B.

AU - Toncelli, A.

AU - Tonelli, M.

AU - Tournefier, E.

AU - Travasso, F.

AU - Trummer, J.

AU - Vajente, G.

AU - van den Brand, J. F.J.

AU - van der Putten, S.

AU - Vavoulidis, M.

AU - Vedovato, G.

AU - Verkindt, D.

AU - Vetrano, F.

AU - Viceré, A.

AU - Vinet, J. Y.

AU - Vocca, H.

AU - Was, M.

AU - Yvert, M.

N1 - Funding Information: The authors gratefully acknowledge the support of the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by the Foundation for Fundamental Research on Matter of the Netherlands Organisation for Scientific Research , the Polish Ministry of Science and Higher Education grant N N203 387237 , the FOCUS Programme of Foundation for Polish Science and the European Associated Laboratory Astrophysics Poland-France.

PY - 2010/3

Y1 - 2010/3

N2 - The performances of the longitudinal sensing and control system of the Virgo gravitational wave detector are described. This system is able to stably maintain the RMS residual fluctuation of the interferometer longitudinal degrees of freedom around or below 10- 11 m, compatible with the original Virgo requirements. Moreover the detector sensitivity is not limited by longitudinal control noise at any frequency. Indeed the noise re-introduced by the longitudinal control system does not affect the Virgo design sensitivity.

AB - The performances of the longitudinal sensing and control system of the Virgo gravitational wave detector are described. This system is able to stably maintain the RMS residual fluctuation of the interferometer longitudinal degrees of freedom around or below 10- 11 m, compatible with the original Virgo requirements. Moreover the detector sensitivity is not limited by longitudinal control noise at any frequency. Indeed the noise re-introduced by the longitudinal control system does not affect the Virgo design sensitivity.

KW - Gravitational waves

KW - Interferometry

KW - Virgo

UR - http://www.scopus.com/inward/record.url?scp=76649136123&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2009.11.006

DO - 10.1016/j.astropartphys.2009.11.006

M3 - Article

AN - SCOPUS:76649136123

SN - 0927-6505

VL - 33

SP - 75

EP - 80

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 2

ER -

Performances of the Virgo interferometer longitudinal control system

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Keywords

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