The third generation of gravitational wave observatories and their science reach

Punturo, M.; R. Abernathy, M.; Acernese, F.; Allen, B.; Andersson, Nils; G. Arun, K.; Barone, F.; Barr, B.; Barsuglia, M.; G. Beker, M.; Beveridge, N.; Birindelli, S.; Bose, S.; Bosi, L.; Braccini, S.; Bradaschia, C.; Bulik, T.; Calloni, E.; Cella, G.; Mottin, Eric; Chelkowski, S.; Chincarini, A.; A. Clark, J.; Coccia, E.; N. Colacino, C.; Colas, J.; Cumming, A.; Cunningham, L.; Cuoco, E.; L. Danilishin, S.; Danzmann, K.; De Luca, Gaetano; De Salvo, R.; Dent, T.; DeRosa, R.; Di Fiore, L.; Di Virgilio, A.; 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, Kostas

doi:10.1088/0264-9381/27/8/084007

Public

The third generation of gravitational wave observatories and their science reach

Shared by NobleBlocks on Apr 6, 2010 • 12:00 AM UTC

Authors:

M. Punturo

M. R. Abernathy

F. Acernese

Abstract

Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced...

Subject

LIGO

Physics

Einstein Telescope

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