Audio-band Coating Thermal Noise Measurement for Advanced LIGO with a Multi-mode Optical Resonator
Abstract
In modern high precision optical instruments, such as in gravitational wave detectors or frequency references, thermally induced fluctuations in the reflective coatings can be a limiting noise source. This noise, known as coating thermal noise, can be reduced by choosing materials with low mechanical loss. Examination of new materials becomes a necessity in order to further minimize the coating thermal noise and thus improve sensitivity of next generation instruments. We present a novel approach to directly measure coating thermal noise using a high finesse folded cavity in which multiple Hermite-Gaussian modes co-resonate. This method is used to probe surface fluctuations on the order 10^-17 m\rtHz in the frequency range 30-400 Hz. We applied this technique to measure thermal noise and loss angle of the coating used in Advanced LIGO.
Keywords
Cite
@article{arxiv.1609.05595,
title = {Audio-band Coating Thermal Noise Measurement for Advanced LIGO with a Multi-mode Optical Resonator},
author = {S. Gras and H. Yu and W. Yam and D. Martynov and M. Evans},
journal= {arXiv preprint arXiv:1609.05595},
year = {2017}
}