Angular Noise in Gravitational Wave Detectors
General Relativity and Quantum Cosmology
2017-08-23 v1
Abstract
Angular fluctuations of suspended mirrors in gravitational wave interferometers are a source of noise both for the locking and the operation of the detectors. We describe here some of the sources of these fluctuations and methods for the estimation of their order of magnitude.
Keywords
Cite
@article{arxiv.gr-qc/0102045,
title = {Angular Noise in Gravitational Wave Detectors},
author = {Gabriela Gonzalez},
journal= {arXiv preprint arXiv:gr-qc/0102045},
year = {2017}
}
Comments
2 pages, to appear in proceedings of the IX Marcel Grossmann meeting, Rome, 2000