Relativistic dust disks and the Wilson-Mathews approach

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dc.creatorKley, Willy
dc.creatorSchaefer, Gerhard
dc.date1998-12-18
dc.date.accessioned2026-07-07T11:46:27Z
dc.date.available2026-07-07T11:46:27Z
dc.descriptionTreating problems in full general relativity is highly complex and frequently approximate methods are employed to simplify the solution. We present comparative solutions of a infinitesimally thin relativistic, stationary, rigidly rotating disk obtained using the full equations and the approximate approach suggested by Wilson & Mathews. We find that the Wilson-Mathews method has about the same accuracy as the first post-Newtonian approximation.
dc.description4 Pages, 5 eps-figures, uses revtex.sty. Submitted to PRL
dc.identifierhttps://arxiv.org/abs/gr-qc/9812068
dc.identifierhttp://arxiv.org/abs/gr-qc/9812068
dc.identifierPhys.Rev.D60:027501,1999
dc.identifierdoi:10.1103/PhysRevD.60.027501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202232
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleRelativistic dust disks and the Wilson-Mathews approach
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