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  • Sathyaprakash, B; Abernathy, M; Allen, B; Barone, F; Barr, B; Bassan, M; Bassiri, R; Beker, M; Beveridge, N; Bizouard, M; Bond, C; Bosi, L; Braccini, S; Bradaschia, C; Brueckner, F; Bulten, H J; Chalkley, E; Chelkowski, S; Clark, J; Corsi, A; Cumming, A; Cuoco, E; De Rosa, R; L Di Fiore; Dietz, A; Doets, M; Edwards, M; Fafone, V; Fairhurst, S; Ferrari, V; Franc, J; Gair, J; Galimberti, M; Genin, E; Glampedakis, K; Graham, W; Hallam, J; Hammond, G; Harms, J; Haughian, K; Hawke, I; Heng, I; Hennes, E; Hough, J; Husa, S; Huttner, S; Iyer, B; Kamaretsos, I; Kawazoe, F; Kley, B; Kumar, R; Lagrange, B; Lastzka, N; Li, T G F; Lück, H; Malvezzi, V; Marion, F; Marque, J; Martin, I; D Mc Leod; Michel, C; Minenkov, Y; Morgia, A; Naticchioni, L; Nawrodt, R; Nelson, J; Ott, C D; Parguez, G; Piergiovanni, F; Pinard, L; Pitkin, M; Plastino, W; Plissi, M; Prato, M; Prodi, G; Rapagnani, P; V Re; Regimbau, T; Ricci, F; Rowan, S; Samblowski, A; Santamaría, L; Schnabel, R; Schwarz, C; Seidel, P; Sopuerta, C F; Sorazu, B; Speirits, F; Strain, K; Tonelli, M; Vaccarone, R; Van Den Broeck, C; van der Putten, S; M van Veggel; Vecchio, A; Vetrano, F; Weßels, P; Willke, B; Winkler, W; Yamamoto, K

    arXiv.org, 06/2012
    Paper, Journal Article

    The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz-10 kHz, with sensitivity a factor ten better in amplitude. Such detectors will be able to probe a range of topics in nuclear physics, astronomy, cosmology and fundamental physics, providing insights into many unsolved problems in these areas.