Site-selection criteria for the Einstein Telescope

The Einstein Telescope (ET) is a proposed next-generation, underground gravitational-wave detector to be based in Europe. It will provide about an order of magnitude sensitivity increase with respect to the currently operating detectors and, also extend the observation band targeting frequencies as...

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Veröffentlicht in:	Review of scientific instruments 2020-09, Vol.91 (9), p.094504-094504
Hauptverfasser:	Amann, Florian, Bonsignorio, Fabio, Bulik, Tomasz, Bulten, Henk Jan, Cuccuru, Stefano, Dassargues, Alain, DeSalvo, Riccardo, Fenyvesi, Edit, Fidecaro, Francesco, Fiori, Irene, Giunchi, Carlo, Grado, Aniello, Harms, Jan, Koley, Soumen, Kovács, László, Losurdo, Giovanni, Mandic, Vuk, Meyers, Patrick, Naticchioni, Luca, Nguyen, Frédéric, Oggiano, Giacomo, Olivieri, Marco, Paoletti, Federico, Paoli, Andrea, Plastino, Wolfango, Razzano, Massimiliano, Ruggi, Paolo, Saccorotti, Gilberto, Sintes, Alicia M., Somlai, László, Ván, Peter, Vasúth, Matyas
Format:	Artikel
Sprache:	eng
Schlagworte:	Background noise Criteria Einstein Telescope Engineering, computing & technology Environmental impact environmental noise Geological, petroleum & mining engineering Gravitational waves Géologie, ingénierie du pétrole & des mines in-depth site Ingénierie, informatique & technologie Noise sensitivity Scientific apparatus & instruments site characterization site selection underground gravitational-wave detector
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