The detection band of the interferometric gravitational wave detector VIRGO can be extended down to a few Hz by suspending each optical component of the interferometer from a chain of mechanical filters designed to suppress the transmission of seismic vibrations. Each mechanical filter supports the weight of the stages below it through a set of cantilevered blade springs. A system of permanent magnets, providing an ''antispring'' force, helps to reduce the highest vertical resonance of the chain from 7 Hz to about 2 Hz. This improvement allows VIRGO to reduce the frequency detection threshold from 10 Hz to about 4 Hz. A characterization of the mechanical filters is provided in this paper.

Extending the VIRGO gravitational wave detection band down to a few Hz: metal blade springs and magnetic antisprings

FERRANTE, ISIDORO;FIDECARO, FRANCESCO;POGGIANI, ROSA;
1997-01-01

Abstract

The detection band of the interferometric gravitational wave detector VIRGO can be extended down to a few Hz by suspending each optical component of the interferometer from a chain of mechanical filters designed to suppress the transmission of seismic vibrations. Each mechanical filter supports the weight of the stages below it through a set of cantilevered blade springs. A system of permanent magnets, providing an ''antispring'' force, helps to reduce the highest vertical resonance of the chain from 7 Hz to about 2 Hz. This improvement allows VIRGO to reduce the frequency detection threshold from 10 Hz to about 4 Hz. A characterization of the mechanical filters is provided in this paper.
1997
Beccaria, M; Bernardini, M; Bougleux, E; Braccini, S; Bradaschia, C; Casciano, C; Cella, G; Cucco, E; Dambrosio, E; Decarolis, G; Delfabbro, R; Desalvo, R; Divirgilio, A; Ferrante, Isidoro; Fidecaro, Francesco; Flaminio, R; Gaddi, A; Gennai, A; Gennaro, G; Giazotto, A; Holoway, L; Lapenna, P; Losurdo, G; Malik, S; Mancini, S; Nicolas, J; Palla, F; Pan, Hb; Paoletti, F; Pasqualetti, A; Passuello, D; Poggiani, Rosa; Popolizio, P; Raffaelli, F; Vicere, A; Waharte, F; Zhang, Z.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/176017
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