Unification of Thermal and Quantum Noises in Gravitational-Wave Detectors

Chris Whittle, Lee McCuller, Vivishek Sudhir, and Matthew Evans
Phys. Rev. Lett. 130, 241401 – Published 12 June 2023

Abstract

Contemporary gravitational-wave detectors are fundamentally limited by thermal noise—due to dissipation in the mechanical elements of the test mass—and quantum noise—from the vacuum fluctuations of the optical field used to probe the test-mass position. Two other fundamental noises can in principle also limit sensitivity: test-mass quantization noise due to the zero-point fluctuation of its mechanical modes and thermal excitation of the optical field. We use the quantum fluctuation-dissipation theorem to unify all four noises. This unified picture shows precisely when test-mass quantization noise and optical thermal noise can be ignored.

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  • Received 23 January 2023
  • Accepted 15 May 2023

DOI:https://doi.org/10.1103/PhysRevLett.130.241401

© 2023 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsQuantum Information, Science & Technology

Authors & Affiliations

Chris Whittle1,*, Lee McCuller2, Vivishek Sudhir1,3,†, and Matthew Evans1

  • 1LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 2LIGO, California Institute of Technology, Pasadena, California 91125, USA
  • 3Department of Mechanical Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139

  • *chris.whittle@ligo.org
  • vivishek@mit.edu

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Vol. 130, Iss. 24 — 16 June 2023

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