The third generation of gravitational wave observatories and their science reach

Autor: By:punturo, M[, 1, 2, ], Abernathy, M[ 3 ], Acernese, Fausto, F[, 4, 5, ], Allen, B[ 6 ], Andersson, N[ 7 ], Arun, K[ 8 ], Barone, Fabrizio, Barr, B[ 3 ], Barsuglia, M[, 9, 10, ], Beker, M[ 11 ], Beveridge, N[ 3 ], Birindelli, S[ 12 ], Bose, S[ 13 ], Bosi, L[ 1 ], Braccini, S[ 14 ], Bradaschia, C[ 14 ], Bulik, T[, 15, 17, 16, 19, 18, 22, ], Calloni, E[, 4, 20, ], Cella, G[ 14 ], Mottin, Ec[, 9, Chelkowski, S[ 21 ], Chincarini, A, Clark, J[ 23 ], Coccia, E[, 24, 25, ], Colacino, C[ 14 ], Colas, J[ 2 ], Cumming, A[ 3 ], Cunningham, L[ 3 ], Cuoco, E[ 2 ], Danilishin, S[ 26 ], Danzmann, K[ 6 ], De Luca, G[ 27 ], De Salvo, R[ 28 ], Dent, T[ 23 ], Derosa, R[, 4, Fiore, Di, L[, 4, Di Virgilio, A[ 14 ], Doets, M[ 11 ], Fafone, V[, 24, Falferi, P[, 29, 30, ], Flaminio, R[ 31 ], Franc, J[ 31 ], Frasconi, F[ 14 ], Freise, A[ 21 ], Fulda, P[ 21 ], Gair, J[ 32 ], Gemme, G, Gennai, A[ 21 ], Giazotto, A[, 2, 14, ], Glampedakis, K[ 33 ], Granata, Grote, H[ 6 ], Guidi, G[, 34, 35, ], Hammond, G[ 3 ], Hannam, M[ 36 ], Harms, J[ 37 ], Heinert, D[ 38 ], Hendry, M[ 3 ], Heng, I[ 3 ], Hennes, E[ 11 ], Hild, S[ 3 ], Hough, J[ 4 ], Husa, S[ 39 ], Huttner, S, Jones, G[ 23 ], Khalili, F[ 40 ], Kokeyama, K[ 21 ], Kokkotas, K[ 33 ], Krishnan, B[ 39 ], Lorenzini, M[ 34 ], Luck, H[ 6 ], Majorana, E[ 41 ], Mandel, I[ 42 ], Mandic, V[ 37 ], Martin, I[ 3 ], Michel, C[ 31 ], Minenkov, Y[, 24, Morgado, N[ 31 ], Mosca, S[, 4, Mours, B[ 43 ], Muller Ebhardt, H[ 6 ], Murray, P[ 3 ], Nawrodt, R[ 3 ], Nelson, J[ 3 ], Oshaughnessy, R[ 44 ], Ott, CD[ 45 ], Palomba, C[ 41 ], Paoli, A[ 2 ], Parguez, G[ 2 ], Pasqualetti, A[ 2 ], Passaquieti, R[, 14, 46, ], Passuello, D[ 14 ], Pinard, L[ 31 ], Poggiani, Popolizio, P[ 2 ], Prato, M, Puppo, P[ 41 ], Rabeling, D[ 11 ], Rapagnani, P[, 41, 47, ], Read, J[ 39 ], Regimbau, T[ 12 ], Rehbein, H[ 6 ], Reid, S[ 3 ], Rezzolla, L[ 39 ], Ricci, F[, 41, Richard, F[ 2 ], Rocchi, A[ 24 ], Rowan, S[ 3 ], Rudiger, A[ 6 ], Sassolas, B[ 31 ], Sathyaprakash, B[ 23 ], Schnabel, R[ 6 ], Schwarz, C[, 48, 49, ], Seidel, P[, 48, Sintes, A[ 39 ], Somiya, K[ 45 ], Speirits, F[ 3 ], Strain, K[ 3 ], Strigin, S[ 40 ], Sutton, P[ 23 ], Tarabrin, S[ 40 ], Van den Brand, J[ 11 ], Van Leewen, C[ 11 ], Van Veggel, M[ 3 ], Van den Broeck, C[ 23 ], Vecchio, A[ 21 ], Veitch, J[ 21 ], Vetrano, F[, 34, Vicere, A[, 34, Vyatchanin, S[ 40 ], Willke, B[ 6 ], Woan, G[ 3 ], Plastino, W[, 49, 50, ], Yamamoto, K.

Publikováno v: Classical and Quantum Gravity
8th Edoardo Amaldi Conference on Gravitational Waves (Amaldi 8)
8th Edoardo Amaldi Conference on Gravitational Waves (Amaldi 8), Jun 2009, New York, United States. pp.084007, ⟨10.1088/0264-9381/27/8/084007⟩
Classical and Quantum Gravity, IOP Publishing, 2010, 27 (8), pp.84007. ⟨10.1088/0264-9381/27/8/084007⟩
Classical and quantum gravity
Classical and Quantum Gravity, 2010, 27 (8), pp.84007. ⟨10.1088/0264-9381/27/8/084007⟩
Classical and Quantum Gravity, 27(8):084007. IOP Publishing Ltd.

Contribution to: 8th Edoardo Amaldi Conference on Gravitational Waves (Amaldi 8); International audience; Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::67b4577be1cf660c50988fd1e1776b48
http://hal.in2p3.fr/in2p3-00472010