Authors
Bangalore Sathyaprakash, Matthew Abernathy, Fausto Acernese, P Ajith, Bruce Allen, P Amaro-Seoane, Nils Andersson, Sofiane Aoudia, K Arun, P Astone, Bala Krishnan, L Barack, Fabrizio Barone, B Barr, M Barsuglia, Massimo Bassan, R Bassiri, Mark Beker, Nicola Beveridge, M Bizouard, C Bond, S Bose, L Bosi, S Braccini, C Bradaschia, M Britzger, F Brueckner, T Bulik, HJ Bulten, O Burmeister, Enrico Calloni, P Campsie, L Carbone, G Cella, E Chalkley, E Chassande-Mottin, S Chelkowski, A Chincarini, A Di Cintio, J Clark, E Coccia, CN Colacino, J Colas, Alberto Colla, A Corsi, A Cumming, L Cunningham, E Cuoco, Stefan Danilishin, K Danzmann, E Daw, R De Salvo, Walter Del Pozzo, Thomas Dent, Rosario De Rosa, L Di Fiore, M Di Paolo Emilio, A Di Virgilio, A Dietz, M Doets, J Dueck, M Edwards, V Fafone, Stephen Fairhurst, P Falferi, M Favata, Valeria Ferrari, F Ferrini, Francesco Fidecaro, R Flaminio, J Franc, F Frasconi, A Freise, D Friedrich, P Fulda, J Gair, M Galimberti, G Gemme, E Genin, A Gennai, A Giazotto, K Glampedakis, S Gossan, R Gouaty, C Graef, W Graham, M Granata, H Grote, GIANLUCA Guidi, J Hallam, G Hammond, Mark Hannam, J Harms, K Haughian, I Hawke, D Heinert, M Hendry, I Heng, E Hennes, S Hild, J Hough, D Huet, S Husa, S Huttner, B Iyer, DI Jones, G Jones, I Kamaretsos, C Kant Mishra, F Kawazoe, F Khalili, B Kley, K Kokeyama, K Kokkotas, S Kroker, R Kumar, K Kuroda, B Lagrange, N Lastzka, TGF Li, M Lorenzini, G Losurdo, H Lück, E Majorana, V Malvezzi, I Mandel, V Mandic, S Marka, F Marin, F Marion, J Marque, I Martin, D Mc Leod, D Mckechan, M Mehmet, Christine Michel, Y Minenkov, N Morgado, A Morgia, S Mosca, L Moscatelli, B Mours, H Müller-Ebhardt, P Murray, Luca Naticchioni, R Nawrodt, J Nelson, R O’Shaughnessy, CD Ott, C Palomba
Publication date
2012/6/1
Journal
Classical and Quantum Gravity
Volume
29
Issue
12
Pages
124013
Publisher
IOP Publishing
Description
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.
Total citations
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Scholar articles
B Sathyaprakash, M Abernathy, F Acernese, P Ajith… - Classical and Quantum Gravity, 2012