作者
Bernard 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, S Bellucci, S Candusso, G Giordano, G Matone, JM Mackowski, L Pinard, Fabrizio Barone, Enrico Calloni, L Di Fiore, M Flagiello, Fabio Garufi, A Grado, Maurizio Longo, M Lops, Stefano Marano, Leopoldo Milano, Salvatore Solimeno, V Brisson, F Cavalier, M Davier, P Hello, P Heusse, P Mann, Y Acker, M Barsuglia, B Bhawal, François Bondu, A Brillet, H Heitmann, JM Innocent, L Latrach, CN Man, M Pham-Tu, E Tournier, M Taubmann, JY Vinet, C Boccara, Ph Gleyzes, V Loriette, JP Roger, G Cagnoli, Luca Gammaitoni, J Kovalik, Fabio Marchesoni, M Punturo, M Beccaria, M Bernardini, E Bougleux, S Braccini, C Bradaschia, G Cella, A Ciampa, E Cuoco, G Curci, R Del Fabbro, R De Salvo, A Di Virgilio, D Enard, Isidoro Ferrante, Francesco Fidecaro, A Giassi, A Giazotto, L Holloway, P La Penna, G Losurdo, S Mancini, Massimo Mazzoni, F Palla, HB Pan, D Passuello, Piergiovanni Pelfer, Rosa Poggiani, Ruggero Stanga, Andrea Vicere, Zhen Zhang, Valeria Ferrari, E Majorana, P Puppo, Piero Rapagnani, Fulvio Ricci
发表日期
1997/6/1
期刊
Classical and Quantum Gravity
卷号
14
期号
6
页码范围
1461
出版商
IOP Publishing
简介
The 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 of a few times 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 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.
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B Caron, A Dominjon, C Drezen, R Flaminio, X Grave… - Classical and Quantum Gravity, 1997