Skip to search
Skip to main content
Back to Search
Start Over
The Einstein Telescope: a third-generation gravitational wave observatory
Authors :
INFN ; INFN European Gravitational Observatory ( EGO ) ; European Gravitational Observatory ( EGO ) Department of Physics and Astronomy ; The University of Glasgow Università di Salerno ; Università di Salerno Max-Planck-Institut ; Max-Planck-Institut University of Southampton ; University of Southampton Université Paris 11, Paris Sud (UP11) ; Université Paris XI - Paris Sud - Ministère de l'Enseignement Supérieur et de la Recherche Scientifique CNRS ; Observatoire de Paris-Université Denis VU University Amsterdam ; CNRS Institut Mondor de Recherche Biomédicale (IMRB) ; INSERM - Université Paris-Est Créteil Val-de-Marne (UPEC) - IFR10 University of Washington ; University of Washington Inst. of Astronomy ; INFN Complesso Universitario di Monte S. Angelo ; Complesso Universitario di Monte S. Angelo University of Birmingham ; University of Birmingham Cardiff University ; Cardiff University Università di Roma Tor ; Università di Roma Tor Moscow State University ; Moscow State University Laboratori Nazionali del Gran Sasso ; Laboratori Nazionali del Gran Sasso LIGO ; California Institute of Technology Sezione di Padova ; Istituto di Fotonica e Nanotecnologie ; INFN, Gruppo Collegato di Trento University of Cambridge (UK) (CAM) ; University of Cambridge (UK) Theoretical Astrophysics ( TAT ) ; Eberhard-Karls-Universität ubingen Università degli Studi di Urbino 'Carlo Bo ' ; Università degli Studi di Urbino 'Carlo Bo ' Department of Physics ; University of Vienna UNIVERSITY OF MINNESOTA ; University of Minnesota Max Planck Institute for Gravitational Physics ( ; Albert Einstein Institute ) Department of Physics and Astronomy ; Northwestern University NSF Astronomy and Astrophysics Postdoctoral Fellow 37 ; Université de Savoie The Pennsylvania State University ; The Pennsylvania State University università di pisa ; Università di Pisa Università degli Studi di Roma "La Sapienza" [Rome] ; Università degli studi di Roma "La Sapienza" Sezione di Roma Tre ; Università di Roma Tre-Dipartimento di Fisica Università degli Studi di Firenze [Firenze] ; Università degli studi di Firenze Punturo, M Abernathy, M Acernese, F Allen, B Andersson, N Arun, K Barone, F Barr, B Barsuglia, M Beker, M Beveridge, N Birindelli, S Bose, S Bosi, L Braccini, S Bradaschia, C Bulik, T Calloni, E Cella, G Mottin, E Chassande Chelkowski, S Chincarini, A Clark, J Coccia, E Colacino, C Colas, J Cumming, A Cunningham, L Cuoco, E Danilishin, S Danzmann, K De Luca, G De Salvo, R Dent, T De Rosa, R Fiore, L Di Virgilio, A Di Doets, M Fafone, V Falferi, P Flaminio, R Franc, J Frasconi, F Freise, A Fulda, P Gair, J Gemme, G Gennai, A Giazotto, A Glampedakis, K Granata, M Grote, H Guidi, G Hammond, G Hannam, M Harms, J Heinert, D Hendry, M Heng, I Hennes, E Hild, S Hough, J Husa, S Huttner, S Jones, G Khalili, F Kokeyama, K Kokkotas, K Krishnan, B Lorenzini, M Uck, H Majorana, E Mandel, I Mandic, V Martin, I Michel, C Minenkov, Y Morgado, N Mosca, S Mours, B Uller-Ebhardt, H Murray, P Nawrodt, R Nelson, J Oshaughnessy, R Ott, C D Palomba, C Paoli, A Parguez, G Pasqualetti, A Passaquieti, R Passuello, D Pinard, L Poggiani, R Popolizio, P Prato, M Puppo, P Rabeling, D Rapagnani, P Read, J Regimbau, T Rehbein, H Reid, S Rezzolla, L Ricci, F Richard, F Rocchi, A Rowan, S Udiger, A Sassolas, B Sathyaprakash, B Schnabel, R Schwarz, C Seidel, P Sintes, A Somiya, K Speirits, F Strain, K Strigin, S Sutton, P Tarabrin, S Uring, A T Van Den Brand, J Van Leewen, C Van Veggel, M Van Den Broeck, C Vecchio, A Veitch, J Vetrano, F Vicere, A Vyatchanin, S Willke, B Woan, G Wolfango, P Yamamoto, K INFN ; INFN European Gravitational Observatory ( EGO ) ; European Gravitational Observatory ( EGO ) Department of Physics and Astronomy ; The University of Glasgow Università di Salerno ; Università di Salerno Max-Planck-Institut ; Max-Planck-Institut University of Southampton ; University of Southampton Université Paris 11, Paris Sud (UP11) ; Université Paris XI - Paris Sud - Ministère de l'Enseignement Supérieur et de la Recherche Scientifique CNRS ; Observatoire de Paris-Université Denis VU University Amsterdam ; CNRS Institut Mondor de Recherche Biomédicale (IMRB) ; INSERM - Université Paris-Est Créteil Val-de-Marne (UPEC) - IFR10 University of Washington ; University of Washington Inst. of Astronomy ; INFN Complesso Universitario di Monte S. Angelo ; Complesso Universitario di Monte S. Angelo University of Birmingham ; University of Birmingham Cardiff University ; Cardiff University Università di Roma Tor ; Università di Roma Tor Moscow State University ; Moscow State University Laboratori Nazionali del Gran Sasso ; Laboratori Nazionali del Gran Sasso LIGO ; California Institute of Technology Sezione di Padova ; Istituto di Fotonica e Nanotecnologie ; INFN, Gruppo Collegato di Trento University of Cambridge (UK) (CAM) ; University of Cambridge (UK) Theoretical Astrophysics ( TAT ) ; Eberhard-Karls-Universität ubingen Università degli Studi di Urbino 'Carlo Bo ' ; Università degli Studi di Urbino 'Carlo Bo ' Department of Physics ; University of Vienna UNIVERSITY OF MINNESOTA ; University of Minnesota Max Planck Institute for Gravitational Physics ( ; Albert Einstein Institute ) Department of Physics and Astronomy ; Northwestern University NSF Astronomy and Astrophysics Postdoctoral Fellow 37 ; Université de Savoie The Pennsylvania State University ; The Pennsylvania State University università di pisa ; Università di Pisa Università degli Studi di Roma "La Sapienza" [Rome] ; Università degli studi di Roma "La Sapienza" Sezione di Roma Tre ; Università di Roma Tre-Dipartimento di Fisica Università degli Studi di Firenze [Firenze] ; Università degli studi di Firenze Punturo, M Abernathy, M Acernese, F Allen, B Andersson, N Arun, K Barone, F Barr, B Barsuglia, M Beker, M Beveridge, N Birindelli, S Bose, S Bosi, L Braccini, S Bradaschia, C Bulik, T Calloni, E Cella, G Mottin, E Chassande Chelkowski, S Chincarini, A Clark, J Coccia, E Colacino, C Colas, J Cumming, A Cunningham, L Cuoco, E Danilishin, S Danzmann, K De Luca, G De Salvo, R Dent, T De Rosa, R Fiore, L Di Virgilio, A Di Doets, M Fafone, V Falferi, P Flaminio, R Franc, J Frasconi, F Freise, A Fulda, P Gair, J Gemme, G Gennai, A Giazotto, A Glampedakis, K Granata, M Grote, H Guidi, G Hammond, G Hannam, M Harms, J Heinert, D Hendry, M Heng, I Hennes, E Hild, S Hough, J Husa, S Huttner, S Jones, G Khalili, F Kokeyama, K Kokkotas, K Krishnan, B Lorenzini, M Uck, H Majorana, E Mandel, I Mandic, V Martin, I Michel, C Minenkov, Y Morgado, N Mosca, S Mours, B Uller-Ebhardt, H Murray, P Nawrodt, R Nelson, J Oshaughnessy, R Ott, C D Palomba, C Paoli, A Parguez, G Pasqualetti, A Passaquieti, R Passuello, D Pinard, L Poggiani, R Popolizio, P Prato, M Puppo, P Rabeling, D Rapagnani, P Read, J Regimbau, T Rehbein, H Reid, S Rezzolla, L Ricci, F Richard, F Rocchi, A Rowan, S Udiger, A Sassolas, B Sathyaprakash, B Schnabel, R Schwarz, C Seidel, P Sintes, A Somiya, K Speirits, F Strain, K Strigin, S Sutton, P Tarabrin, S Uring, A T Van Den Brand, J Van Leewen, C Van Veggel, M Van Den Broeck, C Vecchio, A Veitch, J Vetrano, F Vicere, A Vyatchanin, S Willke, B Woan, G Wolfango, P Yamamoto, K
Source :
Classical and Quantum Gravity; Classical and Quantum Gravity, Institute of Physics: Hybrid Open Access, 2010, 27 (19), pp.194002. <10.1088/0264-9381/27/19/194002>
Abstract
International audience<br />ET: a 3 rd generation GW observatory 2 10 Abstract. Advanced gravitational wave interferometers, currently under realization, will soon permit the detection of gravitational waves from astronomical sources. To open the era of precision gravitational-wave astronomy, a further substantial improvement in sensitivity is required. The future space-based Laser Interferometer Space Antenna (LISA) and the third-generation ground-based observatory Einstein Telescope (ET) promise to achieve the required sensitivity improvements in frequency ranges. The vastly improved sensitivity of the third generation of gravitational-wave observatories could permit detailed measurements of the sources ' physical parameters and could complement, in a multi-messenger approach, the observation of signals emitted by cosmological sources obtained through other kinds of telescopes. This paper describes the progresses of the ET project which is currently in its design study phase. ET: a 3 rd generation GW observatory 3 PACS numbers: 04.80.Nn Submitted to: Class. Quantum Grav. ET: a 3 rd generation GW observatory 4
Details
Database :
OAIster
Journal :
Classical and Quantum Gravity; Classical and Quantum Gravity, Institute of Physics: Hybrid Open Access, 2010, 27 (19), pp.194002. <10.1088/0264-9381/27/19/194002>
Notes :
Classical and Quantum Gravity, English
Publication Type :
Electronic Resource
Accession number :
edsoai.ocn893137651
Document Type :
Electronic Resource