Beyond the Second Generation of Laser-Interferometric Gravitational Wave Observatories
arXiv:1111.6277 · doi:10.1088/0264-9381/29/12/124006
Abstract
This article gives an overview of potential upgrades of second generation gravitational wave detectors and the required key technologies to improve the limiting noise sources. In addition the baseline design of the Einstein Telescope, a European third generation gravitational wave observatory, is briefly discussed.
Amaldi 9 proceedings
Cited by in corpus (28)
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