Scattered light noise in gravitational wave interferometric detectors: Coherent effects

Details Scattered light noise in gravitational wave interferometric detectors: Coherent effects Scattered light noise in gravitational wave interferometric detectors: Coherent effects

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..54.1276v&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 54, Issue 2, 15 July 1996, pp.1276-1286

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18

Gravitational Wave Detectors And Experiments, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

Large interferometric detectors of gravitational waves involve high power light beams stored in optical resonators or Fabry-Perot cavities, installed in km long vacuum pipes. Scattering of light by mirrors, interaction of the scattered light with the walls of the vacuum vessel, and final rescattering on any mirror is a source of noise in such antennas. We present some results obtained within the framework of a coherent approach of scattered light propagation using a coherence function allowing us to study, namely, the effects of small reflecting surfaces along the tube, of diffraction, and of reflection by eventual baffle edges.

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