Impact of upconverted scattered light on advanced interferometric gravitational wave detectors

被引：69

作者：

Ottaway, David J. ^{[1
,2
]}

Fritschel, Peter ^{[3
]}

Waldman, Samuel J. ^{[3
]}

机构：

[1] Univ Adelaide, Dept Phys, Adelaide, SA 5005, Australia

[2] Univ Adelaide, Inst Photon & Adv Sensing, Adelaide, SA 5005, Australia

[3] MIT, Cambridge, MA 02139 USA

来源：

OPTICS EXPRESS | 2012年 / 20卷 / 08期

基金：

美国国家科学基金会;

关键词：

NOISE;

D O I：

10.1364/OE.20.008329

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Second generation gravitational wave detectors are being installed in a number of locations globally. These long-baseline, Michelson interferometers increase the sensitivity between 10 and 40 Hz by many orders of magnitude compared with first generation instruments. Control of non-linear noise coupling from scattered light fields is critical to achieve low frequency performance. In this paper we investigate the requirements on the attenuation of scattered light using a novel time-domain analysis and two years of seismic data from the LIGO Livingston Observatory. (C) 2012 Optical Society of America

引用

页码：8329 / 8336

页数：8

共 19 条

[1] LIGO: the Laser Interferometer Gravitational-Wave Observatory [J].

Abbott, B. P. ;

Abbott, R. ;

Adhikari, R. ;

Ajith, P. ;

Allen, B. ;

Allen, G. ;

Amin, R. S. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arain, M. A. ;

Araya, M. ;

Armandula, H. ;

Armor, P. ;

Aso, Y. ;

Aston, S. ;

Aufmuth, P. ;

Aulbert, C. ;

Babak, S. ;

Baker, P. ;

Ballmer, S. ;

Barker, C. ;

Barker, D. ;

Barr, B. ;

Barriga, P. ;

Barsotti, L. ;

Barton, M. A. ;

Bartos, I. ;

Bassiri, R. ;

Bastarrika, M. ;

Behnke, B. ;

Benacquista, M. ;

Betzwieser, J. ;

Beyersdorf, P. T. ;

Bilenko, I. A. ;

Billingsley, G. ;

Biswas, R. ;

Black, E. ;

Blackburn, J. K. ;

Blackburn, L. ;

Blair, D. ;

Bland, B. ;

Bodiya, T. P. ;

Bogue, L. ;

Bork, R. ;

Boschi, V. ;

Bose, S. ;

Brady, P. R. ;

Braginsky, V. B. ;

Brau, J. E. ;

Bridges, D. O. .

REPORTS ON PROGRESS IN PHYSICS, 2009, 72 (07)

[2] Status of Virgo detector [J].

Acernese, F. ;

Amico, P. ;

Alshourbagy, M. ;

Antonucci, F. ;

Aoudia, S. ;

Astone, P. ;

Avino, S. ;

Babusci, D. ;

Ballardin, G. ;

Barone, F. ;

Barsotti, L. ;

Barsuglia, M. ;

Beauville, F. ;

Bigotta, S. ;

Birindelli, S. ;

Bizouard, M. A. ;

Boccara, C. ;

Bondu, F. ;

Bosi, L. ;

Bradaschia, C. ;

Braccini, S. ;

Brillet, A. ;

Brisson, V. ;

Buskulic, D. ;

Calloni, E. ;

Campagna, E. ;

Carbognani, F. ;

Cavalier, F. ;

Cavalieri, R. ;

Cella, G. ;

Cesarini, E. ;

Chassande-Mottin, E. ;

Christensen, N. ;

Corda, C. ;

Corsi, A. ;

Cottone, F. ;

Clapson, A-C ;

Cleva, F. ;

Coulon, J-P ;

Cuoco, E. ;

Dari, A. ;

Dattilo, V. ;

Davier, M. ;

del Prete, M. ;

De Rosa, R. ;

Di Fiore, L. ;

Di Virgilio, A. ;

Dujardin, B. ;

Eleuteri, A. ;

Ferrante, I. .

CLASSICAL AND QUANTUM GRAVITY, 2007, 24 (19) :S381-S388

[3]

Flanagan E., LIGOT94006300

[4]

Freise A., 2011, COMMUNICATION MAR

[5] Readout and control of a power-recycled interferometric gravitational-wave antenna [J].

Fritschel, P ;

Bork, R ;

González, G ;

Mavalvala, N ;

Ouimette, D ;

Rong, HS ;

Sigg, D ;

Zucker, M .

APPLIED OPTICS, 2001, 40 (28) :4988-4998

[6] Feedforward reduction of the microseism disturbance in a long-base-line interferometric gravitational-wave detector [J].

Giaime, JA ;

Daw, EJ ;

Weitz, M ;

Adhikari, R ;

Fritschel, P ;

Abbott, R ;

Bork, R ;

Heefner, J .

REVIEW OF SCIENTIFIC INSTRUMENTS, 2003, 74 (01) :218-224

[7] Suspensions thermal noise in the LIGO gravitational wave detector [J].

González, G .

CLASSICAL AND QUANTUM GRAVITY, 2000, 17 (21) :4409-4435

[8] Advanced LIGO: the next generation of gravitational wave detectors [J].

Harry, Gregory M. .

CLASSICAL AND QUANTUM GRAVITY, 2010, 27 (08)

[9] Status of LCGT [J].

Kuroda, K. .

CLASSICAL AND QUANTUM GRAVITY, 2010, 27 (08)

[10]

Misner C., 1973, GRAVITATION, P1004

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