Status of the Virgo project

T. Accadia*, F. Acernese, F. Antonucci, P. Astone, G. Ballardin, F. Barone, M. Barsuglia, A. Basti, T.S. Bauer, M. Bebronne, M.G. Beker, A. Belletoile, S. Birindelli, M. Bitossi, M.A. Bizouard, M. Blom, F. Bondu, L. Bonelli, R. Bonnand, V. BoschiL. Bosi, B. Bouhou, S. Braccini, C. Bradaschia, M. Branchesi, T. Briant, A. Brillet, V. Brisson, R. Budzynski, T. Bulik, H.J. Bulten, D. Buskulic, C. Buy, G. Cagnoli, E. Calloni, B. Canuel, F. Carbognani, F. Cavalier, R. Cavalieri, G. Cella, E. Cesarini, O. Chaibi, E.C. Mottin, A. Chincarini, F. Cleva, E. Coccia, P.F. Cohadon, C.N. Colacino, J. Colas, A. Colla, J.F.J. van den Brand

*Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review


We describe the present state and future evolution of the Virgo gravitational wave detector, realized by the Virgo Collaboration at the European Gravitational Observatory, in Cascina near Pisa in Italy. We summarize basic principles of the operation and the design features of the Virgo detector. We present the sensitivity evolution due to a series of intermediate upgrades called Virgo+ which is being completed this year and includes new monolithic suspensions. We describe the present scientific potential of the detector. Finally we discuss the plans for the second generation of the detector, called Advanced Virgo, introducing its new features, the expected sensitivity evolution and the scientific potential.
Original languageEnglish
Article number114002
Number of pages10
JournalClassical and Quantum Gravity
Issue number11
Publication statusPublished - 7 Jun 2011
Externally publishedYes

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