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Determination of the light exposure on the photodiodes of a new instrumented baffle for the Virgo input mode cleaner end-mirror

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arxiv 2008.13740 v2 pith:PGJU4R3X submitted 2020-08-31 physics.ins-det gr-qc

A. Romero , A. Allocca , A. Chiummo , M. Martinez , Ll.M. Mir , H. Yamamoto This is my paper
classification physics.ins-detgr-qc
keywords bafflecleanerinputlightmodephotodiodesend-mirrorexposure
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As part of the upgrade program of the Advanced Virgo interferometer, the installation of new instrumented baffles surrounding the main test masses is foreseen. As a demonstrator, and to validate the technology, the existing baffle in the area of the input mode cleaner end-mirror will be first replaced by a baffle equipped with photodiodes. This paper presents detailed simulations of the light distribution on the input mode cleaner baffle, with the aim to determine the light exposure of the photodiodes under different scenarios of the interferometer operation.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Optomechanical transfer factors for scattered light noise estimations in the beamtubes of ground-based gravitational wave detectors

    gr-qc 2026-07 conditional novelty 6.0 of 10

    Scattered-light noise coupling to strain readout is derived as full optomechanical transfer factors, recovering legacy models only in phase-dominated regimes and substantially revising Einstein Telescope low-frequency...

  2. New modeling of the stray light noise in the main arms of the Einstein Telescope

    physics.ins-det 2025-06 conditional novelty 5.0 of 10

    Stray light noise in Einstein Telescope arms is predicted to stay below the safety margin in ideal conditions, but beam offsets above 4 to 7 cm, tilts above 8 microradians, or strong point absorbers could breach it.

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