New Generation of Superattenuator for Einstein Telescope: preliminary studies
A Bertocco,
M Bruno,
R De Rosa
et al.
Abstract:Seismic noise and local disturbances are dominant noise sources for ground-based Gravitational Waves detectors in the low frequency region (0.1 to 10 Hz) limiting their sensitivity and duty cycle. With the introduction of high-performance seismic isolation systems based on mechanical pendula, the 2nd generation laser interferometric detectors have reached the scientific goal of the first direct observation of GW signals thanks to the extension of the detection bandwidth down to 10 Hz.
Now, the 3rd gene… Show more
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