Precursors of parametric oscillatory instability in LIGO interferometer

被引：11
|
作者：
Polyakov, I. A. [1 ]
Vyatchanin, S. P. [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119992, Russia
来源：
PHYSICS LETTERS A | 2007年 / 368卷 / 06期
基金：
美国国家科学基金会;
关键词：
D O I：
10.1016/j.physleta.2007.04.052
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The basis of undesirable effect of parametric oscillatory instability in optical interferometer is provided by excitation of the additional (Stokes) optical mode having frequency omega(1), and the mirror elastic mode, having frequency omega(m). It appears when optical energy stored in the main mode, with frequency omega(0), exceeds a certain threshold and the frequencies are related as omega(0) similar or equal to omega(1) + omega(m). We analyze the time evolution of parametric instability which allows predicting the characteristics of precursors of parametric instability. Observation of such precursors may help avoid parametric instability. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码：423 / 430
页数：8
相关论文
共 50 条
  • [21] First Demonstration of Electrostatic Damping of Parametric Instability at Advanced LIGO
    Blair, Carl
    Gras, Slawek
    Abbott, Richard
    Aston, Stuart
    Betzwieser, Joseph
    Blair, David
    DeRosa, Ryan
    Evans, Matthew
    Frolov, Valera
    Fritschel, Peter
    Grote, Hartmut
    Hardwick, Terra
    Liu, Jian
    Lormand, Marc
    Miller, John
    Mullavey, Adam
    O'Reilly, Brian
    Zhao, Chunnong
    Abbott, B. P.
    Abbott, T. D.
    Adams, C.
    Adhikari, R. X.
    Anderson, S. B.
    Ananyeva, A.
    Appert, S.
    Arai, K.
    Ballmer, S. W.
    Barker, D.
    Barr, B.
    Barsotti, L.
    Bartlett, J.
    Bartos, I.
    Batch, J. C.
    Bell, A. S.
    Billingsley, G.
    Birch, J.
    Biscans, S.
    Biwer, C.
    Bork, R.
    Brooks, A. F.
    Ciani, G.
    Clara, F.
    Countryman, S. T.
    Cowart, M. J.
    Coyne, D. C.
    Cumming, A.
    Cunningham, L.
    Danzmann, K.
    Costa, C. F. Da Silva
    Daw, E. J.
    PHYSICAL REVIEW LETTERS, 2017, 118 (15)
  • [22] Noise parametric identification and whitening for LIGO 40-m interferometer data
    Cuoco, E
    Losurdo, G
    Calamai, G
    Fabbroni, L
    Mazzoni, M
    Stanga, R
    Guidi, G
    Vetrano, F
    PHYSICAL REVIEW D, 2001, 64 (12)
  • [23] Parametric oscillatory instability in laser gravitational antennas
    Vyatchanin, S. P.
    PHYSICS-USPEKHI, 2012, 55 (03) : 302 - 305
  • [24] Demonstration of dynamic thermal compensation for parametric instability suppression in Advanced LIGO
    Hardwick, T.
    Hamedan, V. J.
    Blair, C.
    Green, A. C.
    Vander-Hyde, D.
    CLASSICAL AND QUANTUM GRAVITY, 2020, 37 (20)
  • [25] Suppression of the Effect of Parametric Instability in the LIGO Voyager Gravitational Wave Detector
    Strigin, S. E.
    MOSCOW UNIVERSITY PHYSICS BULLETIN, 2024, 79 (04) : 462 - 468
  • [26] Parametric oscillatory instability in gravitational wave laser detectors
    Vyatchanin, S. P.
    Strigin, S. E.
    PHYSICS-USPEKHI, 2012, 55 (11) : 1115 - 1123
  • [27] Considerations on parametric instability in Fabry-Perot interferometer
    Kells, W
    D'Ambrosio, E
    PHYSICS LETTERS A, 2002, 299 (04) : 326 - 330
  • [28] Spatiotemporal model of the LIGO interferometer
    Beausoleil, RG
    Sigg, D
    JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION, 1999, 16 (12) : 2990 - 3002
  • [29] Parametric Instability in Advanced Laser Interferometer Gravitational Wave Detectors
    Ju, L.
    Grass, S.
    Zhao, C.
    Degallaix, J.
    Blair, D. G.
    SIXTH EDOARDO AMALDI CONFERENCE ON GRAVITATIONAL WAVES, 2006, 32
  • [30] Suppression of parametric oscillatory instability in third generation gravitational wave detectors
    Strigin, S. E.
    PHYSICS LETTERS A, 2015, 379 (28-29) : 1671 - 1674
12345