Scientific objectives of Einstein Telescope

Sathyaprakash, B ; Abernathy, M ; Acernese, F ; Ajith, P ; Allen, B ; Amaro-Seoane, P ; Andersson, N ; Aoudia, S ; Arun, K ; Astone, P ; Krishnan, B ; Barack, L ; Barone, F ; Barr, B ; Barsuglia, M ; Bassan, M ; Bassiri, R ; Beker, M ; Beveridge, N ; Bizouard, M ; Bond, C ; Bose, S ; Bosi, L ; Braccini, S ; Bradaschia, C ; Britzger, M ; Brueckner, F ; Bulik, T ; Bulten, H J ; Burmeister, O ; Calloni, E ; Campsie, P ; Carbone, L ; Cella, G ; Chalkley, E ; Chassande-Mottin, E ; Chelkowski, S ; Chincarini, A ; Cintio, A Di ; Clark, J ; Coccia, E ; Colacino, C N ; Colas, J ; Colla, A ; Corsi, A ; Cumming, A ; Cunningham, L ; Cuoco, E ; Danilishin, S ; Danzmann, K ; Daw, E ; De Salvo, R ; Pozzo, W Del ; Dent, T ; De Rosa, R ; Fiore, L Di ; Emilio, M Di Paolo ; Virgilio, A Di ; Dietz, A ; Doets, M ; Dueck, J ; Edwards, M ; Fafone, V ; Fairhurst, S ; Falferi, P ; Favata, M ; Ferrari, V ; Ferrini, F ; Fidecaro, F ; Flaminio, R ; Franc, J ; Frasconi, F ; Freise, A ; Friedrich, D ; Fulda, P ; Gair, J ; Galimberti, M ; Gemme, G ; Genin, E ; Gennai, A ; Giazotto, A ; Glampedakis, K ; Gossan, S ; Gouaty, R ; Graef, C ; Graham, W ; Granata, M ; Grote, H ; Guidi, G ; Hallam, J ; Hammond, G ; Hannam, M ; Harms, J ; Haughian, K ; Hawke, I ; Heinert, D ; Hendry, M ; Heng, I ; Hennes, E ; Hild, S ; Hough, J ; Huet, D ; Husa, S ; Huttner, S ; Iyer, B ; Jones, D I ; Jones, G ; Kamaretsos, I ; Mishra, C Kant ; Kawazoe, F ; Khalili, F ; Kley, B ; Kokeyama, K ; Kokkotas, K ; Kroker, S ; Kumar, R ; Kuroda, K ; Lagrange, B ; Lastzka, N ; Li, T G F ; Lorenzini, M ; Losurdo, G ; Lück, H ; Majorana, E ; Malvezzi, V ; Mandel, I ; Mandic, V ; Marka, S ; Marin, F ; Marion, F ; Marque, J ; Martin, I ; Leod, D Mc ; Mckechan, D ; Mehmet, M ; Michel, C ; Minenkov, Y ; Morgado, N ; Morgia, A ; Mosca, S ; Moscatelli, L ; Mours, B ; Müller-Ebhardt, H ; Murray, P ; Naticchioni, L ; Nawrodt, R ; Nelson, J ; Shaughnessy, R O’ ; Ott, C D ; Palomba, C ; Paoli, A ; Parguez, G ; Pasqualetti, A ; Passaquieti, R ; Passuello, D ; Perciballi, M ; Piergiovanni, F ; Pinard, L ; Pitkin, M ; Plastino, W ; Plissi, M ; Poggiani, R ; Popolizio, P ; Porter, E ; Prato, M ; Prodi, G ; Punturo, M ; Puppo, P ; Rabeling, D ; Racz, I ; Rapagnani, P ; Re, V ; Read, J ; Regimbau, T ; Rehbein, H ; Reid, S ; Ricci, F ; Richard, F ; Robinson, C ; Rocchi, A ; Romano, R ; Rowan, S ; Rüdiger, A ; Samblowski, A ; Santamaría, L ; Sassolas, B ; Schilling, R ; Schmidt, P ; Schnabel, R ; Schutz, B ; Schwarz, C ; Scott, J ; Seidel, P ; Sintes, A M ; Somiya, K ; Sopuerta, C F ; Sorazu, B ; Speirits, F ; Storchi, L ; Strain, K ; Strigin, S ; Sutton, P ; Tarabrin, S ; Taylor, B ; Thürin, A ; Tokmakov, K ; Tonelli, M ; Tournefier, H ; Vaccarone, R ; Vahlbruch, H ; van den Brand, J F J ; Van Den Broeck, C ; van der Putten, S ; van Veggel, M ; Vecchio, A ; Veitch, J ; Vetrano, F ; Vicere, A ; Vyatchanin, S ; Weßels, P ; Willke, B ; Winkler, W ; Woan, G ; Woodcraft, A ; Yamamoto, K (2012) Scientific objectives of Einstein Telescope Classical and Quantum Gravity, 29 (12). p. 124013. ISSN 0264-9381

Full text not available from this repository.

Official URL: http://doi.org/10.1088/0264-9381/29/12/124013

Related URL: http://dx.doi.org/10.1088/0264-9381/29/12/124013

Abstract

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 to 10 kHz, with sensitivity a factor 10 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.

Item Type:Article
Source:Copyright of this article belongs to Institute of Physics Publishing.
ID Code:135605
Deposited On:13 Jul 2023 11:20
Last Modified:13 Jul 2023 11:20

Repository Staff Only: item control page