Zobrazeno 1 - 10
of 27
pro vyhledávání: '"di Pace, Sibilla"'
Autor:
Bawaj, Mateusz, Sequino, Valeria, Nguyen, Catherine, Vardaro, Marco, Di Pace, Sibilla, Khan, Imran, Passuello, Diego, Gennai, Alberto, De Laurentis, Martina, Zendri, Jean-Pierre, Sorrentino, Fiodor
In this paper we present a software, developed in the distributed control system environment of the Virgo gravitational-wave detector, for the management of a highly automated optical bench. The bench is extensively used for the research and developm
Externí odkaz:
http://arxiv.org/abs/2004.00316
Autor:
Ast, Stefan, Di Pace, Sibilla, Millo, Jacques, Pichot, Mikhael, Turconi, Margherita, Chaibi, Walid
Publikováno v:
Phys. Rev. D 103, 042008 (2021)
We experimentally demonstrate the conversion of a fundamental $\text{TEM}_{00}$ laser mode at 1064\,nm to higher order Hermite-Gaussian modes (HG) of arbitrary order via a commercially available liquid crystal Spatial Light Modulator (SLM). We partic
Externí odkaz:
http://arxiv.org/abs/1902.01671
Autor:
Khodnevych, Vitalii, Di Pace, Sibilla, Vinet, Jean-Yves, Dinu-Jaeger, Nicoleta, Lintz, Michel
We describe a setup based on Michelson interferometry for coherent measurements of the backscattered light from a low roughness optical surface under test. Special data processing was developed for the extraction of the useful signal from the various
Externí odkaz:
http://arxiv.org/abs/1809.01904
Autor:
Di Pace, Sibilla
L'existence des ondes gravitationnelles (OG) est l'une des prédictions les plus intéressantes de la théorie de la Relativité Générale d'Einstein. La découverte expérimentale des OG serait donc un test important de la théorie elle-même et pe
Externí odkaz:
http://www.theses.fr/2014NICE4108/document
Autor:
Di Pace, Sibilla1,2 (AUTHOR) sibilla.dipace@roma1.infn.it, Naticchioni, Luca2 (AUTHOR), De Laurentis, Martina3 (AUTHOR), Travasso, Flavio4 (AUTHOR)
Publikováno v:
European Physical Journal D (EPJ D). Nov2020, Vol. 74 Issue 11, p1-11. 11p.
A mode cleaner optical cavity is a resonator that can be tuned to transmit a desired transverse mode present in the incoming beam, suppressing all the others. We present the optical design of a suited input mode cleaner for a small-scale Michelson in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b0088ecff69872d1203531eb8db8b53
Autor:
Sequino, Valeria, Barsuglia, Matteo, Bawaj, Mateusz, Bazzan, Marco, Ciani, Giacomo, Conti, Livia, D'Angelo, Beatrice, De Laurentis, Martina, Di Pace, Sibilla, Fafone, Viviana, Garaventa, Barbara, Gennai, Alberto, Giacoppo, Laura, Harms, Jan, Khan, Imran, Naticchioni, Luca, Nguyen, Catherine, Passuello, Diego, Rocchi, Alessio, Sorrentino, Fiodor, Vardaro, Marco, Zendri, Jean-Pierre
Squeezed states of light contribute to the reduction of quantum noise in gravitational-wave interferometers. This result, predicted by Caves in 1981, has been demonstrated by the main gravitational-wave detectors. The injection of phase-squeezed ligh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e0d401d9c51668e0405ec349613c2a8
Autor:
Di Pace, Sibilla, Naticchioni, Luca, Majorana, Ettore, Giacoppo, Laura, Puppo, Paola, Ricci, Fulvio, Rapagnani, Piero, Perciballi, Maurizio, De Laurentis, Martina, Calloni, Enrico, Travasso, Flavio, Bawaj, Mateusz, Vocca, Helios, Piluso, Antonfranco, Sequino, Valeria, Sorrentino, Fiodor
We are developing a small-scale interferometer with monolithic suspension of test masses (SIPS), that will be sensitive to the quantum radiation pressure noise in the audio frequency band of gravitational wave detectors. In the same time, a table-top
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d2c8df80c4e4ab4590952f9ee8e28be
Autor:
Bawaj, Mateusz, De Laurentis, Martina, Di Pace, Sibilla, Gennai, Alberto, Khan, Imran, Majorana, Ettore, Naticchioni, Luca, Nguyen, Catherine, Passuello, Diego, Sequino, Valeria, Sorrentino, Fiodor, Vardaro, Marco, Zendri, Jean-Pierre
In this paper, we introduce the work on hardware and software built to manage the optical bench which hosts the optical squeezer source at the Virgo site in Cascina. In the past, the ex- perimental setup implemented frequency-independent squeezing an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3cbe2229ad485a1daa875a4cddf3c0e0
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