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Sensitivity studies for third-generation gravitational wave observatories

Acernese, F; Barone, F; Beker, M G; Bose, S; Danilishin, S L; Genin, E; Rabeling, David; Sathyaprakash, B; Strigin, S; Yamamoto, K.

Description

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...[Show more]

CollectionsANU Research Publications
Date published: 2011
Type: Journal article
URI: http://hdl.handle.net/1885/72121
Source: Classical and Quantum Gravity
DOI: 10.1088/0264-9381/28/9/094013

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