Optical Interferometers with Reduced Sensitivity to Thermal Noise

H. J. Kimble, Benjamin L. Lev, and Jun Ye
Phys. Rev. Lett. 101, 260602 – Published 30 December 2008

Abstract

A fundamental limit to the sensitivity of optical interferometry is thermal noise that drives fluctuations in the positions of the surfaces of the interferometer’s mirrors, and thereby in the phase of the intracavity field. Schemes for reducing this thermally driven phase noise are presented that rely upon the coherent character of the underlying displacements and strains. Although the position of the physical surface fluctuates, the optical phase upon reflection can have reduced sensitivity to this motion. While practical implementation of such schemes for coherent compensation face certain challenges, we hope to stimulate further work on this important thermal noise problem.

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  • Received 20 June 2008

DOI:https://doi.org/10.1103/PhysRevLett.101.260602

©2008 American Physical Society

Authors & Affiliations

H. J. Kimble*, Benjamin L. Lev, and Jun Ye

  • JILA, National Institute of Standards and Technology and University of Colorado, Boulder, Colorado 80309–0440, USA

  • *Permanent address: California Institute of Technology MC 12-33, Pasadena, CA 91125, USA.
  • Permanent address: Department of Physics, University of Illinois, 1110 West Green Street, Urbana, IL 61801, USA.

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Issue

Vol. 101, Iss. 26 — 31 December 2008

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