EnglishThe Virgo gravitational wave detector is an interferometer with 3 km long arms in construction near Pisa to be commissioned in the year 2000. Virgo has been designed to achieve a strain sensitivity (SNR = 1) of a few times 10(-23) Hz-(1/2) at 200 Hz, A large effort has gone into the conception of the mirror suspension system, which is expected to reduce noise to the level of 10(-21) Hz(-1/2) at 10 HZ. The expected signals and main sources of noise are briefly discussed; the choices made are illustrated together with the present status of the experiment.
| Autori: | |
| Autori: | Caron B; Dominjon A; Drezen C; Flaminio R; Grave X; Marion F; Massonnet L; Mehmel C; Morand R; Mours B; Sannibale V; Yvert M; Babusci D; Bellucci S; Candusso S; Giordano G; Matone G; Mackowski JM; Pinard L; Barone F; Calloni E; DiFiore L; Flagiello M; Garufi F; Grado A; Longo M; Lops M; Marano S; Milano L; Solimeno S; Brisson V; Cavalier F; Davier M; Hello P; Heusse P; Mann P; Acker Y; Barsuglia M; Bhawal B; Bondu F; Brillet A; Heitmann H; Innocent JM; Latrach L; Man CN; PhamTu M; Tournier E; Taubmann M; Vinet JY; Boccara C; Gleyzes P; Loriette V; Roger JP; Cagnoli G; Gammaitoni L; Kovalik J; Marchesoni F; Punturo M; Beccaria M; Bernardini M; Bougleux E; Braccini S; Bradaschia C; Cella G; Ciampa A; Cuoco E; Curci G; DelFabbro R; DeSalvo R; DiVirgilio A; Enard D; Ferrante I; Fidecaro F; Giassi A; Giazotto A; Holloway L; LaPenna P; Losurdo G; Mancini S; Mazzoni M; Palla F; Pan HB; Passuello D; Pelfer P; Poggiani R; Stanga R; Vicere A; Zhang Z; Ferrari V; Majorana E; Puppo P; Rapagnani P; Ricci F |
| Titolo: | The Virgo interferometer RID C-9235-2011 RID B-5375-2009 RID A-1920-2008 |
| Anno del prodotto: | 1997 |
| Appare nelle tipologie: | 1.1 Articolo in rivista |
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http://hdl.handle.net/11568/56503
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