A Nested Inverted Pendulum as a Possible Pre-Isolator for the ET-LF Seismic Isolation System

The third-generation instrument era is approaching, and the Einstein Telescope (ET) giant interferometer is becoming a reality, with the potential to be installed at an underground site where seismic noise is about 100 times lower than at the surface. Moreover, new available technologies and the exp...

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Auteurs principaux:	Lucia Trozzo, Alcide Bertocco, Matteo Bruno, Rosario De Rosa, Luciano Di Fiore, Domenico D’Urso, Franco Frasconi, Alberto Gennai, Leonardo Lucchesi, Moreno Nacca, Federico Pilo, Paolo Prosperi, Davide Rozza, Paolo Ruggi, Valeria Sipala, Francesca Spada
Format:	Artigo
Langue:	Inglês
Publié:	MDPI AG 2025-03-01
Collection:	Galaxies
Sujets:	seismic noise seismic isolation system Einstein Telescope
Accès en ligne:	https://www.mdpi.com/2075-4434/13/2/21
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