The masses used by the Virgo interferometer to detect gravitational waves need adequate isolation from seismic noise. A multistage suspension system has been designed to extend the interferometer sensitivity down around 4 Hz. Motivations for this choice and an outline of the solutions adopted are given.
Suspension of detection masses for the virgo interferometer
FIDECARO, FRANCESCO
1996-01-01
Abstract
The masses used by the Virgo interferometer to detect gravitational waves need adequate isolation from seismic noise. A multistage suspension system has been designed to extend the interferometer sensitivity down around 4 Hz. Motivations for this choice and an outline of the solutions adopted are given.File in questo prodotto:
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