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Each mirror of the interferometric gravitational wave antenna Virgo is attached to a Superattenuator, a chain of mechanical filters designed to suppress seismic vibrations, starting from a few Hz The filter chain attenuation has been measured by exciting its suspension point with sinuisodal forces and using the interferometer as sensor. The attenuation, measured at different frequencies, is compliant with the requirements of the next generation antenna Advanced Virgo In the third generation detector Einstein Telescope, the attenuation is sufficient above 3 Hz, independently of the underground site choice. (C) 2010 Elsevier B.V. All rights reserved.

Measurements of Superattenuator seismic isolation by Virgo interferometer

Acernese F;Antonucci F;Aoudia S;Arun KG;Astone P;Ballardin G;Barone F;Barsuglie M;Bauer TS;Beker MG;Bigotta S;Birindelli S;Bitossi M;Bizouard MA;Blom M;Boccara C;Bondu F;Bonelli L;Bosi L;Braccini S;Bradaschia C;Brillet A;Brisson V;Budzynski R;Bulik T;Bulten HJ;Buskulic D;Cagnoli G;Calloni E;Campagna E;Canuel B;Carbognani F;Cavalier F;Cavalieri R;Celia G;Cesarini E;Chassande Mottin E;Chincarini A;Cleva F;Coccia E;Colacine CN;Colas J;Colla A;Colombini M;Corda C;Corsi A;Coulon JP;Cuoco E;D'Antonio S;Dari A;Dattilo V;Davier M;Day R;De Rosa R;Del Prete M;Di Fiore L;DI LIETO, ALBERTO;Emilio MD;Di Virgilio A;Dietz A;Drago M;Fafone V;FERRANTE, ISIDORO;FIDECARO, FRANCESCO;Fiori I;Flaminio R;Fournier JD;Franc J;Frasca S;Frasconi F;Freise A;Gammaitoni L;Garufi F;Gemme G;Genin E;Gennai A;Giazotto A;Granata M;Greverie C;Guidi G;Heitmann H;Hello P;Hild S;Huet D;Jaranowski P;Kowalska I;Krolak A;La Penna P;Leroy N;Letendre N;Li TGF;Lorenzini M;Loriette V;Losurdo G;Mackowski JM;Majorana E;Man N;Mantovani M;Marchesoni F;Marion F;Marque J;Martelli F;Masserot A;Menzinger F;Michel C;Milano L;Minenkov Y;Mohan M;Moreau J;Morgado N;Morgia A;Mosca S;Moscatelli V;Mours B;Neri I;Nocera F;Pagliaroli G;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, ROSA;Prato M;Prodi GA;Punturo M;Puppo P;Rabaste O;Rabeling DS;Rapagnani P;Re V;Regimbau T;Ricci F;Robinet F;Rocchi A;Rolland L;Romano R;Rosinska D;Ruggi P;Salemi F;Sassolas B;Sentenac D;Sturani R;Swinkels B;TONCELLI, ALESSANDRA;TONELLI, MAURO;Tournefier E;Travasso F;Trummer J;Vajente G;van den Brand JFJ;van der Puttee S;Vavoulidis M;Vedovato G;Verkindt D;Vetrano F;Vicere A;Vinet JY;Vocca H;Was M;Yvert M.

2010-01-01

Abstract

Each mirror of the interferometric gravitational wave antenna Virgo is attached to a Superattenuator, a chain of mechanical filters designed to suppress seismic vibrations, starting from a few Hz The filter chain attenuation has been measured by exciting its suspension point with sinuisodal forces and using the interferometer as sensor. The attenuation, measured at different frequencies, is compliant with the requirements of the next generation antenna Advanced Virgo In the third generation detector Einstein Telescope, the attenuation is sufficient above 3 Hz, independently of the underground site choice. (C) 2010 Elsevier B.V. All rights reserved.

Scheda breve

Scheda completa

Scheda completa (DC)

	Anno
	
			2010
		
	Codice DOI
	
			https://dx.doi.org/10.1016/j.astropartphys.2010.01.006
		
	Tutti gli autori
	
			Acernese, F; Antonucci, F; Aoudia, S; Arun, Kg; Astone, P; Ballardin, G; Barone, F; Barsuglie, M; Bauer, Ts; Beker, Mg; Bigotta, S; Birindelli, S; Bitossi, M; Bizouard, Ma; Blom, M; Boccara, C; Bondu, F; Bonelli, L; Bosi, L; Braccini, S; Bradaschia, C; Brillet, A; Brisson, V; Budzynski, R; Bulik, T; Bulten, Hj; Buskulic, D; Cagnoli, G; Calloni, E; Campagna, E; Canuel, B; Carbognani, F; Cavalier, F; Cavalieri, R; Celia, G; Cesarini, E; Chassande Mottin, E; Chincarini, A; Cleva, F; Coccia, E; Colacine, Cn; Colas, J; Colla, A; Colombini, M; Corda, C; Corsi, A; Coulon, Jp; Cuoco, E; D'Antonio, S; Dari, A; Dattilo, V; Davier, M; Day, R; De Rosa, R; Del Prete, M; Di Fiore, L; DI LIETO, Alberto; Emilio, Md; Di Virgilio, A; Dietz, A; Drago, M; Fafone, V; Ferrante, Isidoro; Fidecaro, Francesco; Fiori, I; Flaminio, R; Fournier, Jd; Franc, J; Frasca, S; Frasconi, F; Freise, A; Gammaitoni, L; Garufi, F; Gemme, G; Genin, E; Gennai, A; Giazotto, A; Granata, M; Greverie, C; Guidi, G; Heitmann, H; Hello, P; Hild, S; Huet, D; Jaranowski, P; Kowalska, I; Krolak, A; La Penna, P; Leroy, N; Letendre, N; Li, Tgf; Lorenzini, M; Loriette, V; Losurdo, G; Mackowski, Jm; Majorana, E; Man, N; Mantovani, M; Marchesoni, F; Marion, F; Marque, J; Martelli, F; Masserot, A; Menzinger, F; Michel, C; Milano, L; Minenkov, Y; Mohan, M; Moreau, J; Morgado, N; Morgia, A; Mosca, S; Moscatelli, V; Mours, B; Neri, I; Nocera, F; Pagliaroli, G; 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, Rosa; Prato, M; Prodi, Ga; Punturo, M; Puppo, P; Rabaste, O; Rabeling, Ds; Rapagnani, P; Re, V; Regimbau, T; Ricci, F; Robinet, F; Rocchi, A; Rolland, L; Romano, R; Rosinska, D; Ruggi, P; Salemi, F; Sassolas, B; Sentenac, D; Sturani, R; Swinkels, B; Toncelli, Alessandra; Tonelli, Mauro; Tournefier, E; Travasso, F; Trummer, J; Vajente, G; van den Brand, Jfj; van der Puttee, S; Vavoulidis, M; Vedovato, G; Verkindt, D; Vetrano, F; Vicere, A; Vinet, Jy; Vocca, H; Was, M; Yvert, M.

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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/190841

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