Compact binary inspiral and the science potential of third-generation ground-based gravitational wave detectors

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dc.creatorBroeck, Chris Van Den
dc.creatorSengupta, Anand S.
dc.date2006-12-13
dc.date.accessioned2026-07-07T07:35:16Z
dc.date.available2026-07-07T07:35:16Z
dc.descriptionWe consider EGO as a possible third-generation ground-based gravitational wave detector and evaluate its capabilities for the detection and interpretation of compact binary inspiral signals. We identify areas of astrophysics and cosmology where EGO would have qualitative advantages, using Advanced LIGO as a benchmark for comparison.
dc.description3 pages, 4 figures. Brief summary of a talk given at the 11th Marcel Grossmann meeting, Berlin, July 2006; to appear in the Proceedings
dc.identifierhttps://arxiv.org/abs/gr-qc/0612085
dc.identifierhttp://arxiv.org/abs/gr-qc/0612085
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120039
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleCompact binary inspiral and the science potential of third-generation ground-based gravitational wave detectors
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