Noise from scattered light in Virgo's second science run data

Autor: Accadia , T, Acernese , F, Antonucci , F, Astone , P, Ballardin , G, Barone , F, Barsuglia , M, Bauer , Th S, Beker , M G, Belletoile , A, Birindelli , S, Bitossi , M, Bizouard , M A, Blom , M, Bondu , François, Bonelli , L, Bonnand , R, Boschi , V, Bosi , L, Bouhou , B, Braccini , S, Bradaschia , C, Brillet , A, Brisson , V, Budzyski , R, Bulik , T, Bulten , H J, Buskulic , D, Lesvigne-Buy , Christelle, Cagnoli , G, Calloni , E, Campagna , E, Canuel , B, Carbognani , F, Cavalier , F, Cavalieri , R, Cella , G, Cesarini , E, Chassande-Mottin , E, Chincarini , A, Cleva , F, Coccia , E, Colacino , C N, Colas , J, Colla , A, Colombini , M, Corsi , A, Coulon , J.-P, Cuoco , E, 9a , Antonio, Dattilo , V, Davier , M, Day , R, 5ab , Rosa, Debreczeni , G, Del , M, 7ac , Prete, Di , L, 5a , Fiore, Di , A, 7ab , Lieto, Di , M, Emilio , Paolo, 7a , Virgilio, Dietz , A, Drago , M, Fafone , V, Ferrante , I, Fidecaro , F, Fiori , I, Flaminio , R, Fournier , J.-D, Franc , J, Frasca , S, Frasconi , F, Freise , A, Galimberti , M, Gammaitoni , L, Garufi , F, Gáspár , M E, Gemme , G, Genin , E, Gennai , A, Giazotto , A, Gouaty , R, Granata , M, Greverie , C, Guidi , G M, Hayau , J.-F, Heitmann , H, Hello , P, Hild , S, Huet , D, Jaranowski , P, Kowalska , I, Królak , A, Leroy , N, Letendre , N, Li , T G F, Lorenzini , M, Loriette , V, Losurdo , G, Majorana , E, Maksimovic , I, Man , N, Mantovani , M, Marchesoni , F, Marion , F, Marque , J, Martelli , F, Masserot , A, Michel , C, Milano , L, Minenkov , Y, Mohan , M, Morgado , N, Morgia , A, Mosca , S, Moscatelli , V, Mours , B, Neri , I, Nocera , F, Pagliaroli , G, Palladino , L, Palomba , C, Paoletti , F, Pardi , S, Parisi , M, Pasqualetti , A, Passaquieti , R, Passuello , D, Persichetti , G, Pichot , M, Piergiovanni , F, Pietka , M, Pinard , L, Poggiani , R, Prato , M, Prodi , G A, Punturo , M, Puppo , P, Rabeling , D S, Rácz , I, Rapagnani , P, Re , V, Regimbau , T, Ricci , F, Robinet , F, Rocchi , A, Rolland , L, Romano , R, Rosiska , D, Ruggi , P, Sassolas , B, Sentenac , D, Sperandio , L, Sturani , R, Swinkels , B L, Toncelli , A, Tonelli , M, Torre , O, Tournefier , E, Travasso , F, Vajente , G, Van Den Brand , J F J, Van Der Putten , S, Vasuth , M, Vavoulidis , M, Vedovato , G, Verkindt , D, Vetrano , F, Viceré , A, Vinet , J.-Y, Vocca , H, Was , M, Yvert , M
Přispěvatelé: ESPCI, Centre National de la Recherche Scientifique ( CNRS ), Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ), INFN, National Institute for Nuclear Physics ( INFN ), European Gravitational Observatory ( EGO ), Institut Mondor de Recherche Biomédicale ( IMRB ), Institut National de la Santé et de la Recherche Médicale ( INSERM ) -IFR10-Université Paris-Est Créteil Val-de-Marne - Paris 12 ( UPEC UP12 ), Nikhef, National institute for Subatomic Physics, Université de Rennes 1 ( UR1 ), Université de Rennes ( UNIV-RENNES ), Sezione di Pisa a, Università degli Studi di Siena ( UNISI ), Université Paris-Sud - Paris 11 ( UP11 ), Institut de Physique de Rennes ( IPR ), Université de Rennes ( UNIV-RENNES ) -Université de Rennes ( UNIV-RENNES ) -Centre National de la Recherche Scientifique ( CNRS ), Università dell'Aquila, INFN, Gruppo Collegato di Trento a and Università di Trento b, Sezione di Padova c, The University of Alabama at Birmingham [ Birmingham] ( UAB ), University of Glasgow, Calloni, Enrico, DE ROSA, Rosario, Forte, LUCA ANTONIO, Garufi, Fabio, Milano, Leopoldo, Mosca, Simona, Pardi, Silvio, Parisi, Maria, G., Persichetti, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry]), Istituto Nazionale di Fisica Nucleare (INFN), European gravitational Observatory (EGO), Istituto Nazionale di Fisica Nucleare (INFN)-Centre National de la Recherche Scientifique (CNRS), Institut Mondor de Recherche Biomédicale (IMRB), Institut National de la Santé et de la Recherche Médicale (INSERM)-IFR10-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12), National Institute for Subatomic Physics [Amsterdam] (NIKHEF), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES), Università degli Studi di Siena = University of Siena (UNISI), Université Paris-Sud - Paris 11 (UP11), Institut de Physique de Rennes (IPR), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Università degli Studi dell'Aquila = University of L'Aquila (UNIVAQ), Università degli Studi di Trento (UNITN), University of Alabama at Birmingham [ Birmingham] (UAB), Université de Rennes (UR), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), (Astro)-Particles Physics
Jazyk: angličtina
Rok vydání: 2010
Předmět:
Zdroj: Classical and Quantum Gravity
14th Gravitational Wave Data Analysis Workshop (GWDAW-14)
14th Gravitational Wave Data Analysis Workshop (GWDAW-14), Jan 2010, rome, Italy. 27 (19), pp.194011, 2010, 〈10.1088/0264-9381/27/19/194011〉
Classical and Quantum Gravity, 27(19):194011. IOP Publishing Ltd.
Accadia, T, Bulten, H J, Rabeling, D S & van den Brand, J F J 2010, ' Noise from scattered light in Virgo's second science run data ', Classical and Quantum Gravity, vol. 27, no. 19, pp. 194011 . https://doi.org/10.1088/0264-9381/27/19/194011
14th Gravitational Wave Data Analysis Workshop (GWDAW-14), Jan 2010, rome, Italy. pp.194011, ⟨10.1088/0264-9381/27/19/194011⟩
Classical and Quantum Gravity, 27(19). IOP Publishing Ltd.
ISSN: 0264-9381
1361-6382
Popis: Virgo is one of the large, ground-based interferometers aimed at detecting gravitational waves. One of the technical problems limiting its sensitivity is caused by light in the output beams which is backscattered by seismically excited surfaces and couples back into the main beam of the interferometer. The resulting noise was thoroughly studied, measured and mitigated before Virgo's second science run (VSR2). The residual noise during VSR2, which increases in periods with a large microseism activity, is accurately predicted by the theoretical model. The scattered light has been associated with transient events in the gravitational-wave signal of the interferometer. © 2010 IOP Publishing Ltd.
Databáze: OpenAIRE
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