158 articles – 1990 Notices  [english version]
 HAL : in2p3-00588056, version 1
 arXiv : 1012.0908
 8th International LISA Symposium, Stanford : États-Unis (2010)
 Sensitivity Studies for Third-Generation Gravitational Wave Observatories
 (2011)
 Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.
 équipe(s) de recherche : APC - Cosmologie et GravitationAPC - ADAMIS
 Thème(s) : Physique/Relativité Générale et Cosmologie Quantique
 Lien vers le texte intégral : http://fr.arXiv.org/abs/1012.0908
 in2p3-00588056, version 1 http://hal.in2p3.fr/in2p3-00588056 oai:hal.in2p3.fr:in2p3-00588056 Contributeur : Françoise Marechal <> Soumis le : Vendredi 22 Avril 2011, 10:46:58 Dernière modification le : Jeudi 21 Juin 2012, 17:45:30