Measurement of the VIRGO superattenuator performance for seismic noise suppression

被引:93
作者
Ballardin, G
Bracci, L [1 ]
Braccini, S
Bradaschia, C
Casciano, C
Calamai, G
Cavalieri, R
Cecchi, R
Cella, G
Cuoco, E
D'Ambrosio, E
Dattilo, V
Di Virgilio, A
Fabbroni, L
Fidecaro, F
Frasconi, F
Gaddi, A
Gennai, A
Gennaro, G
Giazotto, A
Losurdo, G
Holloway, L
La Penna, P
Lelli, F
Majorana, E
Mazzoni, M
Paoletti, F
Pasotti, M
Pasqualetti, A
Passaquieti, R
Passuello, D
Poggiani, R
Puppo, P
Raffaelli, F
Rapagnani, P
Ricci, F
Ruggi, P
Stanga, R
Taddei, R
Vetrano, F
Vicerè, A
Zhang, Z
机构
[1] Ist Nazl Fis Nucl, VIRGO Project, Sez Pisa, Pisa, Italy
[2] Univ Pisa, Dipartimento Fis, I-56100 Pisa, Italy
[3] Osserv Astrofis Arcetri, I-50125 Florence, Italy
[4] Ist Nazl Fis Nucl, VIRGO Project, Sez Firenze, Florence, Italy
[5] Univ Florence, Dipartimento Astron, I-50121 Florence, Italy
[6] Ist Nazl Fis Nucl, VIRGO Project, Sez Roma, Rome, Italy
[7] Univ Roma 1, Dipartimento Fis, Rome, Italy
[8] Univ Urbino, Dipartimento Fis, I-61029 Urbino, Italy
关键词
D O I
10.1063/1.1392338
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
Below a few tens of hertz interferometric detection of gravitational waves is masked by seismic vibrations of the optical components. In order to isolate the mirrors of the VIRGO interferometer, a sophisticated suspension system, called superattenuator, has been developed. Its working principle is based on a multistage pendulum acting on seismic vibrations as a chain of second order mechanical low-pass filters. A complete superattenuator has been built and tested. This apparatus allows extending the VIRGO detection band down to a few Hz. A detailed description of the attenuation system and its performance are presented in this article. (C) 2001 American Institute of Physics.
引用
收藏
页码:3643 / 3652
页数:10
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