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Journal of the Optical Society of America A

Journal of the Optical Society of America A

| OPTICS, IMAGE SCIENCE, AND VISION

  • Vol. 17, Iss. 1 — Jan. 1, 2000
  • pp: 120–128

Analysis of light noise sources in a recycled Michelson interferometer with Fabry–Perot arms

J. B. Camp, H. Yamamoto, S. E. Whitcomb, and D. E. McClelland  »View Author Affiliations


JOSA A, Vol. 17, Issue 1, pp. 120-128 (2000)
http://dx.doi.org/10.1364/JOSAA.17.000120


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Abstract

We present a method by which the effect of laser field variations on the signal output of an interferometric gravitational wave detector is rigorously determined. Using the Laser Interferometer Gravitational Wave Observatory (LIGO) optical configuration of a power recycled Michelson interferometer with Fabry–Perot arm cavities as an example, we calculate the excess noise after the input filter cavity (mode cleaner) and the dependence of the detector strain sensitivity on laser frequency and amplitude noise, radio frequency oscillator noise, and scattered-light phase noise. We find that noise on the radio frequency sidebands generally limits the detector’s sensitivity.

© 2000 Optical Society of America

OCIS Codes
(120.2230) Instrumentation, measurement, and metrology : Fabry-Perot
(120.3180) Instrumentation, measurement, and metrology : Interferometry

Citation
J. B. Camp, H. Yamamoto, S. E. Whitcomb, and D. E. McClelland, "Analysis of light noise sources in a recycled Michelson interferometer with Fabry–Perot arms," J. Opt. Soc. Am. A 17, 120-128 (2000)
http://www.opticsinfobase.org/josaa/abstract.cfm?URI=josaa-17-1-120


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References

  1. A. Abramovici, W. Althouse, R. W. P. Drever, Y. Gursel, S. Kawamura, F. J. Raab, D. Shoemaker, L. Sievers, R. E. Spero, R. E. Vogt, R. Weiss, S. E. Whitcomb, and M. E. Zucker, “LIGO: The Laser Interferometer Gravitational-Wave Observatory,” Science 256, 325–333 (1992).
  2. A. Giazotto, “The VIRGO experiment: status of the art,” in First Edoardo Amaldi Conference on Gravitational Wave Experiments, E. Coccia, G. Pizella, and F. Ronga, eds. (World Scientific, Singapore, 1995), pp. 86–99.
  3. K. Tsubono, “300-m laser interferometer gravitational wave detector (TAMA300) in Japan,” in First Edoardo Amaldi Conference on Gravitational Wave Experiments, E. Coccia, G. Pizella, and F. Ronga, eds. (World Scientific, Singapore, 1995), pp. 112–114.
  4. K. Danzmann, “GEO600—a 600 m laser interferometric gravitational wave antenna,” in First Edoardo Amaldi Conference on Gravitational Wave Experiments, E. Coccia, G. Pizella, and F. Ronga, eds. (World Scientific, Singapore, 1995), pp. 100–111.
  5. R. W. P. Drever, J. L. Hall, F. V. Kowalski, J. Hough, G. M. Ford, A. J. Munley, and H. Ward, “Laser phase and frequency stabilization using an optical resonator,” Appl. Phys. B 31, 97–105 (1983).
  6. R. Drever, in Quantum Optics, Experimental Gravity and Measurement Theory, P. Meystre and M. Scully, eds. (Plenum, New York, 1983), pp. 503–514.
  7. A. Siegman, Lasers (University Science, Mill Valley, Calif., 1986), Chap. 11.
  8. M. Regehr, “Signal extraction and control for an interferometric gravitational wave detector,” Ph.D. dissertation (California Institute of Technology, Pasadena, Calif., 1995).
  9. K. D. Skeldon and K. A. Strain, “Response of a Fabry–Perot optical cavity to phase-modulation sidebands for use in electro-optic control systems,” Appl. Opt. 36, 6802–6808 (1997).
  10. S. Whitcomb, “Optics Development for LIGO,” in Proceedings of the TAMA International Workshop on Gravitational Wave Detection, K. Tsubono, M.-K. Fujimoto, and K. Kuroda, eds. (Universal Academy Press, Tokyo, 1996), pp. 229–239.
  11. Marconi model 2023.
  12. D. E. McClelland, J. B. Camp, J. Mason, W. Kells, and S. E. Whitcomb, “Arm cavity resonant sideband control for laser interferometric gravitational wave detectors,” Opt. Lett. 24, 1014–1016 (1999).

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