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Measurement of the Stray Light in the Advanced Virgo Input Mode Cleaner Cavity using an instrumented baffle

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arxiv 2111.09312 v2 pith:CQ4QFYZZ submitted 2021-11-17 astro-ph.IM gr-qc

classification astro-ph.IMgr-qc
keywords cavitybaffleinputlightvirgocleanerdatainstrumented
verification ladder T0 review T1 audit T2 compute T3 formal
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A new instrumented baffle was installed in Spring 2021 at Virgo surrounding the suspended mirror in the input mode cleaner triangular cavity. It serves as a demonstrator of the technology designed to instrument the baffles in the main arms in the near future. We present, for the first time, results on the measured scattered light distribution inside the cavity as determined by the new device using data collected between May and July 2021, with Virgo in commissioning phase and operating with an input laser power in the cavity of 28.5~W. The sensitivity of the baffle is discussed and the data is compared to scattered light simulations.

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Cited by 1 Pith paper

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

  1. Advanced Virgo during the LIGO-Virgo-KAGRA fourth observing run

    gr-qc 2026-07 accept novelty 4.0 of 10

    Virgo completed dual recycling for O4 but was limited by nearly unstable cavities and unidentified excess noise, yielding 68.9% duty cycle and 53 Mpc BNS range after SR misalignment.

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