Listening for Ringing Black Holes

Simple item page
dc.creatorCreighton, Jolien D. E.
dc.date1997-12-10
dc.date.accessioned2026-07-07T03:32:06Z
dc.date.available2026-07-07T03:32:06Z
dc.descriptionThe gravitational radiation produced by binary black holes during their inspiral, merger, and ringdown phases is a promising candidate for detection by the first or second generation of kilometer-scale interferometric gravitational wave antennas. Waveforms for the last phase, the quasinormal ringing, are well understood. I discuss the feasibility of detection of the quasinormal ringing of a black hole based on an analysis of the Caltech 40-meter interferometer data.
dc.description8 pages LaTeX, 1 eps figure included with epsfig, based on a talk given at the 7th Canadian Conference on General Relativity and Relativistic Astrophysics
dc.identifierhttps://arxiv.org/abs/gr-qc/9712044
dc.identifierhttp://arxiv.org/abs/gr-qc/9712044
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36100
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleListening for Ringing Black Holes
dc.typetext

Files

Collections

arXiv