Lock acquisition of the central interferometer of the gravitational wave detector Virgo

被引:5
作者
Acernese, F
Amico, P
Arnaud, N
Babusci, D
Barillé, R
Barone, F
Barsotti, L
Barsuglia, M
Beauville, F
Bracci, L
Braccini, S
Brillet, A
Brisson, V
Brocco, L
Buskulic, D
Calamai, G
Calloni, E
Campagna, E
Cavalier, F
Cella, G
Chassande-Mottin, E
Cleva, F
Cokelaer, T
Corda, C
Coulon, JP
Cuoco, E
Dattilo, V
Davier, M
De Rosa, R
Di Fiore, L
Di Virgilio, A
Dujardin, B
Eleuteri, A
Enard, D
Ferrante, I
Fidecaro, F
Fiori, I
Flaminio, R
Fournier, JD
Frasca, S
Frasconi, F
Gammaitoni, L
Gennai, A
Giazotto, A
Giordano, G
Guidi, G
Heitmann, H
Hello, P
Heusse, P
Holloway, L
机构
[1] Univ Paris 11, CNRS, IN2P3, LAL, F-91898 Orsay, France
[2] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[3] Univ Perugia, I-06123 Perugia, Italy
[4] Univ Salerno, I-84084 Salerno, Italy
[5] Univ Naples Federico II, I-80126 Naples, Italy
[6] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy
[7] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
[8] EGO, I-56021 Cascina, PI, Italy
[9] Univ Pisa, I-56127 Pisa, Italy
[10] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[11] Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France
[12] ESPCI, F-75005 Paris, France
[13] Observ Cote Azur, Dept Fresnel Interferometrie Laser Gravitat & Ast, F-06304 Nice 4, France
[14] Ist Nazl Fis Nucl, Sez Firenzel Urbino, I-50019 Sesto Fiorentino, Italy
[15] Univ Florence, I-50125 Florence, Italy
[16] Osserv Astrofis Arcetri, I-50125 Florence, Italy
[17] Univ Urbino, I-61029 Urbino, Italy
[18] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[19] Univ Roma La Sapienza, I-00185 Rome, Italy
[20] SMA, IPNL 22, F-69622 Villeurbanne, France
关键词
gravitational waves detectors; interferometer; control systems; servo and control equipment;
D O I
10.1016/j.astropartphys.2004.03.007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the lock acquisition algorithm used for the central interferometer of the gravitational wave detector Virgo (CITF). The CITF was a preliminary step in the construction of the Virgo detector, which allowed to test the main components of the instrument. The problems related to the lock acquisition are discussed, together with the key points of the algorithm. Computer simulation in the time domain of the detector was crucial to develop and test the algorithm. A comparison between simulation of the lock acquisition and the corresponding experimental results is shown. (C) 2004 Elsevier B.V. All rights reserved.
引用
收藏
页码:465 / 477
页数:13
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