The oscillation and stability of differentially rotating spherical shells: The normal mode problem

Simple item page
dc.creatorWatts, Anna L.
dc.creatorAndersson, Nils
dc.creatorBeyer, Horst
dc.creatorSchutz, Bernard F.
dc.date2002-10-04
dc.date2003-04-29
dc.date.accessioned2026-07-07T12:27:41Z
dc.date.available2026-07-07T12:27:41Z
dc.descriptionAn understanding of the dynamics of differentially rotating systems is key to many areas of astrophysics. We investigate the oscillations of a simple system exhibiting differential rotation, and discuss issues concerning the role of corotation points and the emergence of dynamical instabilities. This problem is of particular relevance to the emission of gravitational waves from oscillating neutron stars, which are expected to possess significant differential rotation immediately after birth or binary merger.
dc.description14 pages, 6 figures, minor error corrected, MNRAS in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0210122
dc.identifierhttp://arxiv.org/abs/astro-ph/0210122
dc.identifierMon.Not.Roy.Astron.Soc.342:1156,2003
dc.identifierdoi:10.1046/j.1365-8711.2003.06612.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215288
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe oscillation and stability of differentially rotating spherical shells: The normal mode problem
dc.typetext

Files

Collections

arXiv