作者
S Hild, M Abernathy, F ea Acernese, P Amaro-Seoane, N Andersson, K Arun, F Barone, B Barr, M Barsuglia, M Beker, N Beveridge, S Birindelli, S Bose, L Bosi, S Braccini, C Bradaschia, T Bulik, E Calloni, G Cella, E Chassande Mottin, S Chelkowski, A Chincarini, J Clark, Eugenio Coccia, C Colacino, J Colas, A Cumming, L Cunningham, E Cuoco, Stefan Danilishin, K Danzmann, R De Salvo, Thomas Dent, R De Rosa, L Di Fiore, A Di Virgilio, M Doets, Viviana Fafone, P Falferi, R Flaminio, J Franc, F Frasconi, A Freise, D Friedrich, P Fulda, J Gair, G Gemme, E Genin, A Gennai, A Giazotto, K Glampedakis, C Gräf, M Granata, H Grote, GIANLUCA Guidi, A Gurkovsky, G Hammond, Mark Hannam, J Harms, D Heinert, M Hendry, I Heng, E Hennes, J Hough, S Husa, S Huttner, Geraint Jones, F Khalili, K Kokeyama, K Kokkotas, B Krishnan, TGF Li, M Lorenzini, H Lück, E Majorana, I Mandel, V Mandic, M Mantovani, I Martin, Christine Michel, Y Minenkov, N Morgado, S Mosca, B Mours, H Müller–Ebhardt, P Murray, R Nawrodt, J Nelson, R Oshaughnessy, CD Ott, C Palomba, A Paoli, G Parguez, A Pasqualetti, Roberto Passaquieti, D Passuello, L Pinard, W Plastino, Rosa Poggiani, P Popolizio, M Prato, M Punturo, P Puppo, D Rabeling, P Rapagnani, J Read, T Regimbau, H Rehbein, S Reid, F Ricci, F Richard, A Rocchi, S Rowan, A Rüdiger, L Santamaría, B Sassolas, B Sathyaprakash, R Schnabel, C Schwarz, P Seidel, A Sintes, K Somiya, F Speirits, K Strain, S Strigin, P Sutton, S Tarabrin, A Thüring, J van Den Brand, M Van Veggel, C van Den Broeck, A Vecchio, John Veitch, Flavio Vetrano, Andrea Vicere, S Vyatchanin, B Willke, G Woan, K Yamamoto
发表日期
2011/4/18
期刊
Classical and Quantum gravity
卷号
28
期号
9
页码范围
094013
出版商
IOP Publishing
简介
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.
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S Hild, M Abernathy, F Acernese, P Amaro-Seoane… - Classical and Quantum gravity, 2011