English

Fluctuation-dissipation theorem for thermo-refractive noise

Statistical Mechanics 2009-11-13 v1 Astrophysics General Relativity and Quantum Cosmology

Abstract

We introduce a simple prescription for calculating the spectra of thermal fluctuations of temperature-dependent quantities of the form δT^(t)=d3rδT(r,t)q(r)\hat{\delta T}(t)=\int d^3\vec{r} \delta T(\vec{r},t) q(\vec{r}). Here T(r,t)T(\vec{r}, t) is the local temperature at location r\vec{r} and time tt, and q(r)q(\vec{r}) is an arbitrary function. As an example of a possible application, we compute the spectrum of thermo-refractive coating noise in LIGO, and find a complete agreement with the previous calculation of Braginsky, Gorodetsky and Vyatchanin. Our method has computational advantage, especially for non-regular or non-symmetric geometries, and for the cases where q(r)q(\vec{r}) is non-negligible in a significant fraction of the total volume.

Keywords

Cite

@article{arxiv.0710.2710,
  title  = {Fluctuation-dissipation theorem for thermo-refractive noise},
  author = {Yuri Levin},
  journal= {arXiv preprint arXiv:0710.2710},
  year   = {2009}
}

Comments

3 pages

R2 v1 2026-06-21T09:31:37.907Z