Sensitivity studies for third-generation gravitational wave observatories

Hild, S.; Abernathy, M. R.; Acernese, F.; Amaro‐Seoane, Pau; Andersson, Nils; Arun, K. G.; Barone, F.; Barr, B.; Barsuglia, M.; Beker, M. G.; Beveridge, N.; Birindelli, S.; Bose, S.; Bosi, L.; Braccini, S.; Bradaschia, C.; Bulik, T.; Calloni, E.; Cella, G.; Mottin, Eric; Chelkowski, S.; Chincarini, A.; Clark, J. A.; Coccia, E.; Colacino, C. N.; Colas, J.; Cumming, A.; Cunningham, L.; Cuoco, E.; Danilishin, S. L.; Danzmann, K.; Salvo, R. De; Dent, T.; Rosa, R. De; Fiore, L. Di; Virgilio, A. Di; Doets, M.; Fafone, V.; Falferi, P.; Flaminio, R.; Franc, J.; Frasconi, F.; Freise, A.; Friedrich, Daniel; Fulda, P.; Gair, J.; Gemme, G.; Genin, É.; Gennai, A.; Giazotto, A.; Glampedakis, Kostas; Gräf, Christian; Granata, M.; Grote, H.; Guidi, G. M.; Gurkovsky, A. G.; Hammond, G.; Hannam, M; Harms, J.; Heinert, D.; Hendry, M.; Heng, I. S.; Hennes, E.; Hough, J.; Husa, S.; Huttner, S. H.; Jones, Gareth; Khalili, F. Y.; Kokeyama, K.; Kokkotas, Kostas D.; Krishnan, B.; Li, T.G.F.; Lorenzini, M.; Lück, H.; Majorana, E.; Mandel, Ilya; Mandic, V.; Mantovani, M.; Martin, I. W.; Michel, C.; Minenkov, Y.; Morgado, N.; Mosca, S.; Mours, B.; Müller‐Ebhardt, H.; Murray, P. G.; Nawrodt, R.; Nelson, John H.; O’Shaughnessy, R.; Ott, C. D.; Palomba, C.; Paoli, A.; Parguez, G; Pasqualetti, A.; Passaquieti, R.; Passuello, D.; Pinard, L.; Plastino, W.; Poggiani, R.; Popolizio, P.; Prato, Mirko; Punturo, M.; Puppo, P.; Rabeling, D. S.; Rapagnani, P.; Read, J.; Regimbau, T.; Rehbein, H.; Reid, S.; Ricci, F; Richard, F; Rocchi, A.; Rowan, S.; Rüdiger, A.; Santamaría, L.; Sassolas, B.; Sathyaprakash, B. S.; Schnabel, R.; Schwarz, Christian; Seidel, P.; Sintes, A. M.; Somiya, K.; Speirits, F. C.; Strain, K. A.; Strigin, S.; Sutton, P. J.; Tarabrin, S. P.; Thüring, A.; Brand, J. F. J. van den; Veggel, M van; Broeck, C van den; Vecchio, A.; Veitch, J.; Vetrano, F.; Viceré, A.; Vyatchanin, S.; Willke, B.; Woan, G.; Yamamoto, Kazuhiro

doi:10.1088/0264-9381/28/9/094013

articleClassical and Quantum GravityApr 19, 2011BRONZE OA

Sensitivity studies for third-generation gravitational wave observatories

SHS. Hild MRM. R. Abernathy FAF. Acernese PAPau Amaro‐Seoane NANils Andersson

University of Glasgow · University of Salerno · +46 more institutions

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Abstract

Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex Class. Quantum Grav. 28 (2011) 094013 S Hild et al mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate…

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Topics & keywords

Topics

Keywords

Gravitational wave
Physics
Einstein Telescope
Detector
Gravitational-wave observatory
Noise (video)
Sensitivity (control systems)
Gravitational field

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