The intermediate problem for binary black hole inspiral and the periodic standing wave approximation

Simple item page
dc.creatorBromley, Benjamin
dc.creatorOwen, Robert
dc.creatorPrice, Richard H.
dc.date2005-02-28
dc.date.accessioned2026-07-07T03:29:26Z
dc.date.available2026-07-07T03:29:26Z
dc.descriptionIn calculations of the inspiral of binary black holes an intermediate approximation is needed that can bridge the post-Newtonian methods of the early inspiral and the numerical relativity computations of the final plunge. We describe here the periodic standing wave approximation: A numerical solution is found to the problem of a periodic rotating binary with helically symmetric standing wave fields, and from this solution an approximation is extracted for the physically relevant problem of inspiral with outgoing waves. The approximation underlying this approach has been recently confirmed with innovative numerical methods applied to nonlinear model problems.
dc.description4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0502121
dc.identifierhttp://arxiv.org/abs/gr-qc/0502121
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35217
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe intermediate problem for binary black hole inspiral and the periodic standing wave approximation
dc.typetext

Files

Collections

arXiv