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Instrumented baffle for the Advanced Virgo input mode cleaner end mirror

A novel instrumented baffle surrounding the suspended end mirror in the input mode cleaner cavity of the Virgo interferometer was installed in Spring 2021. Since then, the device has been regularly operated in the experiment, and the data collected show good stability. The baffle will operate in the...

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Detalles Bibliográficos
Autores principales: Andrés-Carcasona, M., Ballester, O., Blanch, O., Campos, J., Caneva, G., Cardiel, L., Cavalli-Sforza, M., Chiggiato, P., Chiummo, A., Ferreira, J.A., Illa, J.M., Karathanasis, C., Kolstein, M., Martínez, M., Macquet, A., Menendez-Vázquez, A., Mir, Ll.M., Mundet, J., Pasqualetti, A., Piccinni, O., Pio, C., Romero-Rodríguez, A., Serrano, D., Dattilo, V.
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.107.062001
http://cds.cern.ch/record/2853497
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author Andrés-Carcasona, M.
Ballester, O.
Blanch, O.
Campos, J.
Caneva, G.
Cardiel, L.
Cavalli-Sforza, M.
Chiggiato, P.
Chiummo, A.
Ferreira, J.A.
Illa, J.M.
Karathanasis, C.
Kolstein, M.
Martínez, M.
Macquet, A.
Menendez-Vázquez, A.
Mir, Ll.M.
Mundet, J.
Pasqualetti, A.
Piccinni, O.
Pio, C.
Romero-Rodríguez, A.
Serrano, D.
Dattilo, V.
author_facet Andrés-Carcasona, M.
Ballester, O.
Blanch, O.
Campos, J.
Caneva, G.
Cardiel, L.
Cavalli-Sforza, M.
Chiggiato, P.
Chiummo, A.
Ferreira, J.A.
Illa, J.M.
Karathanasis, C.
Kolstein, M.
Martínez, M.
Macquet, A.
Menendez-Vázquez, A.
Mir, Ll.M.
Mundet, J.
Pasqualetti, A.
Piccinni, O.
Pio, C.
Romero-Rodríguez, A.
Serrano, D.
Dattilo, V.
author_sort Andrés-Carcasona, M.
collection CERN
description A novel instrumented baffle surrounding the suspended end mirror in the input mode cleaner cavity of the Virgo interferometer was installed in Spring 2021. Since then, the device has been regularly operated in the experiment, and the data collected show good stability. The baffle will operate in the upcoming O4 observation run, serving as a demonstrator of the technology designed to instrument the baffles in front of the main mirrors in time for O5. In this paper, we present a detailed description of the baffle design, including mechanics, front-end electronics, and data acquisition as well as optical and vacuum compatibility tests, calibration and installation procedures, and performance results.
id cern-2853497
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2022
record_format invenio
spelling cern-28534972023-06-21T02:42:09Zdoi:10.1103/PhysRevD.107.062001http://cds.cern.ch/record/2853497engAndrés-Carcasona, M.Ballester, O.Blanch, O.Campos, J.Caneva, G.Cardiel, L.Cavalli-Sforza, M.Chiggiato, P.Chiummo, A.Ferreira, J.A.Illa, J.M.Karathanasis, C.Kolstein, M.Martínez, M.Macquet, A.Menendez-Vázquez, A.Mir, Ll.M.Mundet, J.Pasqualetti, A.Piccinni, O.Pio, C.Romero-Rodríguez, A.Serrano, D.Dattilo, V.Instrumented baffle for the Advanced Virgo input mode cleaner end mirrorgr-qcGeneral Relativity and Cosmologyastro-ph.IMAstrophysics and Astronomyphysics.ins-detDetectors and Experimental TechniquesA novel instrumented baffle surrounding the suspended end mirror in the input mode cleaner cavity of the Virgo interferometer was installed in Spring 2021. Since then, the device has been regularly operated in the experiment, and the data collected show good stability. The baffle will operate in the upcoming O4 observation run, serving as a demonstrator of the technology designed to instrument the baffles in front of the main mirrors in time for O5. In this paper, we present a detailed description of the baffle design, including mechanics, front-end electronics, and data acquisition as well as optical and vacuum compatibility tests, calibration and installation procedures, and performance results.A novel instrumented baffle surrounding the suspended end mirror in the input mode cleaner cavity of the Virgo interferometer was installed in spring 2021. Since then, the device has been regularly operated in the experiment and the obtained results indicate a good agreement with simulations of the stray light inside the optical cavity. The baffle will operate in the upcoming O4 observation run, serving as a demonstrator of the technology designed to instrument the baffles in front of the main mirrors in time for O5. In this paper we present a detailed description of the baffle design, including mechanics, front-end electronics, data acquisition, as well as optical and vacuum tests, calibration and installation procedures, and performance results.arXiv:2210.16313oai:cds.cern.ch:28534972022-10-27
spellingShingle gr-qc
General Relativity and Cosmology
astro-ph.IM
Astrophysics and Astronomy
physics.ins-det
Detectors and Experimental Techniques
Andrés-Carcasona, M.
Ballester, O.
Blanch, O.
Campos, J.
Caneva, G.
Cardiel, L.
Cavalli-Sforza, M.
Chiggiato, P.
Chiummo, A.
Ferreira, J.A.
Illa, J.M.
Karathanasis, C.
Kolstein, M.
Martínez, M.
Macquet, A.
Menendez-Vázquez, A.
Mir, Ll.M.
Mundet, J.
Pasqualetti, A.
Piccinni, O.
Pio, C.
Romero-Rodríguez, A.
Serrano, D.
Dattilo, V.
Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title_full Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title_fullStr Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title_full_unstemmed Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title_short Instrumented baffle for the Advanced Virgo input mode cleaner end mirror
title_sort instrumented baffle for the advanced virgo input mode cleaner end mirror
topic gr-qc
General Relativity and Cosmology
astro-ph.IM
Astrophysics and Astronomy
physics.ins-det
Detectors and Experimental Techniques
url https://dx.doi.org/10.1103/PhysRevD.107.062001
http://cds.cern.ch/record/2853497
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