Performance of an instrumented baffle placed at the entrance of Virgo's end mirror vacuum tower during O5
Abstract
In this article, we present results on the simulated performance of an instrumented baffle installed at the entrance of the vacuum towers hosting the end mirrors of Virgo’s main Fabry-Pérot cavities. The installation of instrumented baffles is part of the Advanced Virgo Plus upgrade in time for the O5 observing run. They were originally envisaged to be suspended, mounted on new payloads and surrounding new larger end mirrors. The current Virgo upgrade plan includes the replacement of the mirrors with new ones of better quality and same dimensions, leaving the installation of new payloads and larger end mirrors to a post-O5 upgrade phase still to be defined. Here we demonstrate that placing the instrumented baffles just beyond the cryotrap gate valve and in front of the end mirrors would be equally effective for monitoring scattered light inside the cavities. This new location, more than a meter away from the mirror, further reduces the risk of contamination and any potential interference with the mirrors, preserves the full capability to monitor scattered light, and decouples the instrumented baffle timeline from the plans for installing large mirrors in the experiment. We provide an estimate of the light distribution the baffles would encounter under both nominal and non-nominal conditions, as well as an assessment of the scattered light noise introduced by these baffles in this new location, confirming that they would not compromise Virgo’s sensitivity.
Copyright and License
© 2025 American Physical Society.
Acknowledgement
This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 754510. This work is partially supported by the Spanish MCIN/AEI/10.13039/501100011033 under the Grants No. SEV-2016-0588, No. PGC2018-101858-B, No. PID2020-113701GB-I00, and No. PID2023-146517NB-I00 some of which include ERDF funds from the European Union, and by the MICINN with funding from the European Union NextGenerationEU (PRTR-C17.I1) and by the Generalitat de Catalunya. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. M. A. C. is supported by AGAUR (Generalitat de Catalunya) 2022 Grant No. FI-00335. Part of this material is based upon work supported by NSF’s LIGO Laboratory which is a major facility fully funded by the National Science Foundation and operates under Cooperative Agreement No. PHY-1764464.
Data Availability
The data supporting this study’s findings are available within the article.
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Additional details
- European Commission
- 754510
- Ministerio de Ciencia, Innovación y Universidades
- Agencia Estatal de Investigación
- SEV-2016-0588
- Agencia Estatal de Investigación
- PGC2018-101858-B
- Agencia Estatal de Investigación
- PID2020–113701 GB-I00
- Agencia Estatal de Investigación
- PID2023-146517NB-I00
- European Commission
- PRTR-C17.I1
- Government of Catalonia
- Agència de Gestió d'Ajuts Universitaris i de Recerca
- FI-00335
- CERCA Institution
- National Science Foundation
- PHY-1764464
- Accepted
-
2025-01-13Accepted
- Caltech groups
- LIGO
- Publication Status
- Published