Scattered light noise in gravitational wave interferometric detectors: A statistical approach

Details Scattered light noise in gravitational wave interferometric detectors: A statistical approach Scattered light noise in gravitational wave interferometric detectors: A statistical approach

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvd..56.6085v&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 56, Issue 10, 15 November 1997, pp.6085-6095

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11

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

Scientific paper

The sensitivity of interferometric detectors of gravitational waves such as LIGO or VIRGO could eventually be limited by the noise due to scattered light propagation and rescattering in the long vacuum pipes containing the laser beams. We propose a statistical method for evaluating scattered light noise and compare trapping systems, easy to implement in Monte Carlo simulation codes.

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