Details
Original language | English |
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Pages | 137-144 |
Number of pages | 8 |
Publication status | Published - 2011 |
Event | 46th Rencontres de Moriond and GPhyS Colloquium on Gravitational Waves and Experimental Gravity 2011 - La Thuile, Italy Duration: 20 Mar 2011 → 27 Mar 2011 |
Conference
Conference | 46th Rencontres de Moriond and GPhyS Colloquium on Gravitational Waves and Experimental Gravity 2011 |
---|---|
Country/Territory | Italy |
City | La Thuile |
Period | 20 Mar 2011 → 27 Mar 2011 |
Abstract
Interferometric gravitational wave detectors currently under operation have reached their design sensitivities and will by upgraded to their second generation having ten times more sensitivity. It is expected that these instruments will detect gravitational waves directly for the first time and thus opening the era of gravitational wave astronomy. The Einstein Telescope design study - funded by the European Commission - investigates the technical and scientific challenges for a third generation of gravitational wave detectors that will have a 100 times better sensitivity compared to the first generation. This contribution summarises selected experimental approaches for the Einstein Telescope and will discuss challenges for the future research within this vital field of precision measurements.
ASJC Scopus subject areas
- Engineering(all)
- General Engineering
- Mathematics(all)
- Applied Mathematics
- Mathematics(all)
- Modelling and Simulation
- Physics and Astronomy(all)
- General Physics and Astronomy
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2011. 137-144 Paper presented at 46th Rencontres de Moriond and GPhyS Colloquium on Gravitational Waves and Experimental Gravity 2011, La Thuile, Italy.
Research output: Contribution to conference › Paper › Research › peer review
}
TY - CONF
T1 - Experimental approaches for the Einstein Telescope
AU - Nawrodt, R.
AU - Abernathy, M.
AU - Acernese, F.
AU - Amaro-Seoane, P.
AU - Andersson, N.
AU - Arun, K.
AU - Barone, F.
AU - Barr, B.
AU - Barsuglia, M.
AU - Beker, M.
AU - Beveridge, N.
AU - Birindelli, S.
AU - Bose, S.
AU - Bosi, L.
AU - Braccini, S.
AU - Bradaschia, C.
AU - Bulik, T.
AU - Calloni, E.
AU - Cella, G.
AU - Chassande Mottin, E.
AU - Chelkowski, S.
AU - Chincarini, A.
AU - Clark, J.
AU - Coccia, E.
AU - Colacino, C.
AU - Colas, J.
AU - Cumming, A.
AU - Cunningham, L.
AU - Cuoco, E.
AU - Danilishin, S.
AU - Danzmann, K.
AU - DeSalvo, R.
AU - Dent, T.
AU - DeRosa, R.
AU - DiFiore, L.
AU - Di Virgilio, A.
AU - Doets, M.
AU - Fafone, V.
AU - Falferi, P.
AU - Flaminio, R.
AU - Franc, J.
AU - Frasconi, F.
AU - Freise, A.
AU - Friedrich, D.
AU - Fulda, P.
AU - Gair, J.
AU - Gemme, G.
AU - Genin, E.
AU - Gennai, A.
AU - Giazotto, A.
AU - Glampedakis, K.
AU - Gräf, C.
AU - Granata, M.
AU - Grote, H.
AU - Guidi, G.
AU - Gurkovsky, A.
AU - Hammond, G.
AU - Hannam, M.
AU - Harms, J.
AU - Heinert, D.
AU - Hendry, M.
AU - Heng, I.
AU - Hennes, E.
AU - Hild, S.
AU - Hough, J.
AU - Husa, S.
AU - Huttner, S.
AU - Jones, G.
AU - Khalili, F.
AU - Kokeyama, K.
AU - Kokkotas, K.
AU - Krishnan, B.
AU - Li, T. G.F.
AU - Lorenzini, M.
AU - Lück, H.
AU - Majorana, E.
AU - Mandel, I.
AU - Mandic, V.
AU - Mantovani, M.
AU - Martin, I.
AU - Michel, C.
AU - Minenkov, Y.
AU - Morgado, N.
AU - Mosca, S.
AU - Mours, B.
AU - Müller-Ebhardt, H.
AU - Murray, P.
AU - Nelson, J.
AU - Oshaughnessy, R.
AU - Ott, C. D.
AU - Palomba, C.
AU - Paoli, A.
AU - Parguez, G.
AU - Pasqualetti, A.
AU - Passaquieti, R.
AU - Passuello, D.
AU - Pinard, L.
AU - Plastino, W.
AU - Poggiani, R.
AU - Popolizio, P.
AU - Prato, M.
AU - Punturo, M.
AU - Puppo, P.
AU - Rabeling, D.
AU - Racz, I.
AU - Rapagnani, P.
AU - Read, J.
AU - Regimbau, T.
AU - Rehbein, H.
AU - Reid, S.
AU - Rezzolla, L.
AU - Ricci, F.
AU - Richard, F.
AU - Rocchi, A.
AU - Rowan, S.
AU - Rüdiger, A.
AU - Santamaría, L.
AU - Sassolas, B.
AU - Sathyaprakash, B.
AU - Schnabel, R.
AU - Schwarz, C.
AU - Seidel, P.
AU - Sintes, A.
AU - Somiya, K.
AU - Speirits, F.
AU - Strain, K.
AU - Strigin, S.
AU - Sutton, P.
AU - Tarabrin, S.
AU - Thüring, A.
AU - Van Den Brand, J.
AU - Van Veggel, M.
AU - Van Den Broeck, C.
AU - Vecchio, A.
AU - Veitch, J.
AU - Vetrano, F.
AU - Vicere, A.
AU - Vyatchanin, S.
AU - Willke, B.
AU - Woan, G.
AU - Yamamoto, K.
N1 - Funding Information: The authors would like to thank the European Commission for the financial support under the Framework Programme 7 (FP7) 'Capacities' - project Einstein Telescope (ET) design study (Grant Agreement 211743). RN acknowledges the support of the German Science Foundation under contract SFB TR7. Funding Information: The authors would like to thank the European Commission for the financial support under the Framework Programme 7 (FP7) ’Capacities’ - project Einstein Telescope (ET) design study (Grant Agreement 211743). RN acknowledges the support of the German Science Foundation under contract SFB TR7. Publisher Copyright: © Thê Gioi Publishers, 2011.
PY - 2011
Y1 - 2011
N2 - Interferometric gravitational wave detectors currently under operation have reached their design sensitivities and will by upgraded to their second generation having ten times more sensitivity. It is expected that these instruments will detect gravitational waves directly for the first time and thus opening the era of gravitational wave astronomy. The Einstein Telescope design study - funded by the European Commission - investigates the technical and scientific challenges for a third generation of gravitational wave detectors that will have a 100 times better sensitivity compared to the first generation. This contribution summarises selected experimental approaches for the Einstein Telescope and will discuss challenges for the future research within this vital field of precision measurements.
AB - Interferometric gravitational wave detectors currently under operation have reached their design sensitivities and will by upgraded to their second generation having ten times more sensitivity. It is expected that these instruments will detect gravitational waves directly for the first time and thus opening the era of gravitational wave astronomy. The Einstein Telescope design study - funded by the European Commission - investigates the technical and scientific challenges for a third generation of gravitational wave detectors that will have a 100 times better sensitivity compared to the first generation. This contribution summarises selected experimental approaches for the Einstein Telescope and will discuss challenges for the future research within this vital field of precision measurements.
UR - http://www.scopus.com/inward/record.url?scp=85091485058&partnerID=8YFLogxK
M3 - Paper
AN - SCOPUS:85091485058
SP - 137
EP - 144
T2 - 46th Rencontres de Moriond and GPhyS Colloquium on Gravitational Waves and Experimental Gravity 2011
Y2 - 20 March 2011 through 27 March 2011
ER -