Angular Noise in Gravitational Wave Detectors

Details Angular Noise in Gravitational Wave Detectors Angular Noise in Gravitational Wave Detectors

2001-02-11

arxiv.org/abs/gr-qc/0102045v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

2 pages, to appear in proceedings of the IX Marcel Grossmann meeting, Rome, 2000

Scientific paper

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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