Angular Noise in Gravitational Wave Detectors
广义相对论与量子宇宙学
2017-08-23 v1
摘要
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.
引用
@article{arxiv.gr-qc/0102045,
title = {Angular Noise in Gravitational Wave Detectors},
author = {Gabriela Gonzalez},
journal= {arXiv preprint arXiv:gr-qc/0102045},
year = {2017}
}
备注
2 pages, to appear in proceedings of the IX Marcel Grossmann meeting, Rome, 2000