The VIRGO interferometer for gravitational wave detection

B Caron,A Dominjon,C Drezen,R Flaminio,X Grave,F Marion,L Massonnet,C Mehmel,R Morand,B Mours,V Sannibale,M Yvert,D Babusci,Stefano Bellucci, S Candusso, G Giordano,G Matone,J M Mackowski,L Pinard,Fabrizio Barone,E Calloni,L Di Fiore,M Flagiello, F Garuti,A Grado,Michael J Longo,Marco Lops,Stefano Marano,L Milano,S Solimeno,V Brisson,F Cavalier,M Davier,P Hello, P Heusse,P Mann, Y Acker,M Barsuglia,B Bhawal,F Bondu,A Brillet,H Heitmann,J M Innocent, L Latrach,C N Man, M Phamtu,E Tournier, M Taubmann,J Y Vinet,C Boccara,Ph Gleyzes,V Loriette, J P Roger,G Cagnoli,L Gammaitoni,J Kovalik,Fabio Marchesoni,M Punturo,Matteo Beccaria,M Bernardini, E Bougleux,S Braccini,C Bradaschia,G Cella, A Ciampa,E Cuoco, Giuseppe Curci,R Del Fabbro,R De Salvo,A Di Virgilio, D Enard,I Ferrante,F Fidecaro, A Giassi,A Giazotto,L Holloway,P La Penna,G Losurdo,Stefano Mancini,M A Mazzoni,F Palla,H B Pan,D Passuello,P G Pelfer,R Poggiani, R Stanga,A Vicere,Zhiming Zhang,Vittorio Ferrari,E Majorana,P Puppo,P Rapagnani,F Ricci

Nuclear Physics B - Proceedings Supplements（1997）

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摘要

The Virgo gravitational wave detector is an interferometer with 3 km long arms in construction near Pisa in Italy. The accessible sources at the design sensitivity and main noises are reviewed. Virgo has devoted a significant effort to extend sensitivity to low frequency reaching the strain level (h) over tilde = 10(-21) Hz(-1/2) at 10 Hz while at 200 Hz (h) over tilde = 3.10(-23) Hz(-1/2). Design choices and status of construction are presented.

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