Angular Noise in Gravitational Wave Detectors
Gabriela Gonzalez (Center for Gravitational Physics, Geometry, The, Pennsylvania State University)
TL;DR
This paper discusses the sources and estimation methods of angular noise in suspended mirrors of gravitational wave detectors, highlighting its impact on detector operation and stability.
Contribution
It provides an analysis of angular fluctuation sources and introduces methods to estimate their magnitude in gravitational wave interferometers.
Findings
Identified key sources of angular noise.
Developed estimation techniques for angular fluctuations.
Implications for improving detector stability.
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.
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Taxonomy
TopicsGeophysics and Sensor Technology · Pulsars and Gravitational Waves Research · Advanced Frequency and Time Standards