The gravitational wave detector Advanced Virgo+ is currently in the commissioning phase in view of the fourth Observing Run (O4). The major upgrades with respect to the Advanced Virgo configuration are the implementation of an additional recycling cavity, the Signal Recycling cavity (SRC), at the output of the interferometer to broaden the sensitivity band and the Frequency Dependent Squeezing (FDS) to reduce quantum noise at all frequencies. The main difference of the Advanced Virgo + detector with respect to the LIGO detectors is the presence of marginally stable recycling cavities, with respect to the stable recycling cavities present in the LIGO detectors, which increases the difficulties in controlling the interferometer in presence of defects (both thermal and cold defects). This work will focus on the interferometer commissioning, highlighting the control challenges to maintain the detector in the working point which maximizes the sensitivity and the duty cycle for scientific data taking.
The Advanced Virgo+ status / F. Acernese, M. Agathos, A. Ain, S. Albanesi, C. Allene, A. Allocca, A. Amato, M. Andia, T. Andrade, N. Andres, M. Andres-Carcasona, T. Andric, S. Ansoldi, S. Antier, T. Apostolatos, E.Z. Appavuravther, M. Arene, N. Arnaud, M. Assiduo, S.A.D.S. Melo, P. Astone, F. Aubin, S. Babak, F. Badaracco, S. Bagnasco, J. Baird, T. Baka, G. Ballardin, G. Baltus, B. Banerjee, P. Barneo, F. Barone, M. Barsuglia, D. Barta, A. Basti, M. Bawaj, M. Bazzan, F. Beirnaert, M. Bejger, V. Benedetto, M. Berbel, S. Bernuzzi, D. Bersanetti, A. Bertolini, U. Bhardwaj, A. Bianchi, M. Bilicki, S. Bini, M. Bischi, M. Bitossi, M.-. Bizouard, F. Bobba, M. Boer, G. Bogaert, G. Boileau, M. Boldrini, L.D. Bonavena, R. Bondarescu, F. Bondu, R. Bonnand, V. Boschi, V. Boudart, Y. Bouffanais, A. Bozzi, C. Bradaschia, M. Braglia, M. Branchesi, M. Breschi, T. Briant, A. Brillet, J. Brooks, G. Bruno, F. Bucci, O. Bulashenko, T. Bulik, H.J. Bulten, R. Buscicchio, D. Buskulic, C. Buy, G. Cabras, R. 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Girolamo, D. Diksha, A.D. Lieto, A.D. Michele, S.D. Pace, I.D. Palma, F.D. Renzo, L. D'Onofrio, T. Dooney, O. Dorosh, M. Drago, J.-. Ducoin, U. Dupletsa, O. Durante, D. D'Urso, P.-. Duverne, L. Errico, D. Estevez, F. Fabrizi, F. Faedi, V. Fafone, G. Favaro, M. Fays, E. Fenyvesi, I. Ferrante, F. Fidecaro, P. Figura, A. Fiori, I. Fiori, R. Fittipaldi, V. Fiumara, R. Flaminio, J.A. Font, S. Frasca, F. Frasconi, A. Freise, O. Freitas, G.G. Fronze, B. Gadre, R. Gamba, B. Garaventa, J. Garcia-Bellido, J. Gargiulo, F. Garufi, C. Gasbarra, G. Gemme, A. Gennai, A. Ghosh, L. Giacoppo, P. Giri, F. Gissi, S. Gkaitatzis, F. Glotin, B. Goncharov, M. Gosselin, R. Gouaty, A. Grado, M. Granata, V. Granata, G. Greco, G. Grignani, A. Grimaldi, D. Guerra, D. Guetta, G.M. Guidi, F. Gulminelli, Y. Guo, P. Gupta, N. Gutierrez, L. Haegel, O. Halim, O. Hannuksela, T. Harder, K. Haris, T. Harmark, J. Harms, B. Haskell, A. Heidmann, H. Heitmann, P. Hello, G. Hemming, E. Hennes, J.-. Hennig, M. Hennig, S. 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Tamanini, A.J. Tanasijczuk, E.N. Tapia San Martin, C. Taranto, M. Tonelli, A. Torres-Forne, I.T.E. Melo, E. Tournefier, A. Trapananti, F. Travasso, J. Trenado, M.C. Tringali, L. Troiano, A. Trovato, L. Trozzo, K.W. Tsang, K. Turbang, M. Turconi, C. Turski, H. Ubach, A. Utina, M. Valentini, S. Vallero, N. Van Bakel, M. Van Beuzekom, M. Van Dael, J.F.J. Van Den Brand, C. Van Den Broeck, M. Van Der Sluys, A. Van De Walle, J. Van Dongen, H. Van Haevermaet, J.V. Van Heijningen, Z. Van Ranst, N. Van Remortel, M. Vardaro, M. Vasuth, G. Vedovato, P. Verdier, D. Verkindt, P. Verma, F. Vetrano, A. Vicere, J.-. Vinet, S. Viret, A. Virtuoso, H. Vocca, R.C. Walet, M. Was, N. Yadav, A. Zadroa1/4ny, T. Zelenova, J.-. Zendri. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6588. - 2429:1(2023), pp. 012039.1-012039.13. (Intervento presentato al 12. convegno CRIS Cosmic Ray International Seminar : September, 12-16 tenutosi a Napoli nel 2022) [10.1088/1742-6596/2429/1/012039].
The Advanced Virgo+ status
B. Haskell;
2023
Abstract
The gravitational wave detector Advanced Virgo+ is currently in the commissioning phase in view of the fourth Observing Run (O4). The major upgrades with respect to the Advanced Virgo configuration are the implementation of an additional recycling cavity, the Signal Recycling cavity (SRC), at the output of the interferometer to broaden the sensitivity band and the Frequency Dependent Squeezing (FDS) to reduce quantum noise at all frequencies. The main difference of the Advanced Virgo + detector with respect to the LIGO detectors is the presence of marginally stable recycling cavities, with respect to the stable recycling cavities present in the LIGO detectors, which increases the difficulties in controlling the interferometer in presence of defects (both thermal and cold defects). This work will focus on the interferometer commissioning, highlighting the control challenges to maintain the detector in the working point which maximizes the sensitivity and the duty cycle for scientific data taking.File | Dimensione | Formato | |
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