The variable finesse locking technique

被引:23
作者
Acernese, F. [1 ]
Amico, P.
Al-Shourbagy, M.
Aoudia, S.
Avino, S.
Babusci, D.
Ballardin, G.
Barille, R.
Barone, F.
Barsotti, L.
Barsuglia, M.
Beauville, F.
Bizouard, M. A.
Boccara, C.
Bosi, L.
Bradaschia, C.
Braccini, S.
Brillet, A.
Brisson, V.
Brocco, L.
Buskulic, D.
Calloni, E.
Campagna, E.
Cavalier, F.
Cavalieri, R.
Cella, G.
Chassande-Mottin, E.
Corda, C.
Clapson, A. -C.
Cleva, F.
Coulon, J. -P.
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, J. -D.
Frasca, S.
Frasconi, F.
Freise, A.
Gammaitoni, L.
Gennai, A.
机构
[1] Ist Nazl Fis Nucl, Sez Napoli, I-80125 Naples, Italy
[2] Univ Naples Federico II, Naples, Italy
[3] Univ Salerno, Fisciano, SA, Italy
[4] Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy
[5] Univ Perugia, I-06100 Perugia, Italy
[6] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy
[7] Univ Pisa, Pisa, Italy
[8] Observ Cote Azur, Dept Artemis, F-06304 Nice 4, France
[9] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, RM, Italy
[10] European Gravitat Observ, Cascina, PI, Italy
[11] Univ Paris 11, CNRS, IN2P3, LAL, Orsay, France
[12] Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France
[13] ESPCI, F-75005 Paris, France
[14] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy
[15] Univ Roma La Sapienza, Rome, Italy
[16] Ist Nazl Fis Nucl, Sez Firenze, Urbino, Sesto Fiorenti, Italy
[17] Univ Florence, I-50121 Florence, Italy
[18] Univ Urbino, I-61029 Urbino, Italy
[19] LMA, Lyon, France
[20] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
关键词
D O I
10.1088/0264-9381/23/8/S12
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Virgo is a power recycled Michelson interferometer, with 3 km long Fabry-Perot cavities in the arms. The locking of the interferometer has been obtained with an original lock acquisition technique. The main idea is to lock the instrument away from its working point. Lock is obtained by misaligning the power recycling mirror and detuning the Michelson from the dark fringe. In this way, a good fraction of light escapes through the antisymmetric port and the power build-up inside the recycling cavity is extremely low. The benefit is that all the degrees of freedom are controlled when they are almost decoupled, and the linewidth of the recycling cavity is large. The interferometer is then adiabatically brought on to the dark fringe. This technique is referred to as variable finesse, since the recycling cavity is considered as a variable finesse Fabry-Perot. This technique has been widely tested and allows us to reach the dark fringe in few minutes, in an essentially deterministic way.
引用
收藏
页码:S85 / S89
页数:5
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