On the steady states of the spherically symmetric Einstein-Vlasov system

dc.creatorAndreasson, Hakan
dc.creatorRein, Gerhard
dc.date2006-11-08
dc.date.accessioned2026-07-07T10:21:59Z
dc.date.available2026-07-07T10:21:59Z
dc.descriptionUsing both numerical and analytical tools we study various features of static, spherically symmetric solutions of the Einstein-Vlasov system. In particular, we investigate the possible shapes of their mass-energy density and find that they can be multi-peaked, we give numerical evidence and a partial proof for the conjecture that the Buchdahl inequality $\sup_{r > 0} 2 m(r)/r < 8/9$, $m(r)$ the quasi-local mass, holds for all such steady states--both isotropic {\em and} anisotropic--, and we give numerical evidence and a partial proof for the conjecture that for any given microscopic equation of state--both isotropic {\em and} anisotropic--the resulting one-parameter family of static solutions generates a spiral in the radius-mass diagram.
dc.description34 pages, 18 figures, LaTex
dc.identifierhttps://arxiv.org/abs/gr-qc/0611053
dc.identifierhttp://arxiv.org/abs/gr-qc/0611053
dc.identifierClass.Quant.Grav.24:1809-1832,2007
dc.identifierdoi:10.1088/0264-9381/24/7/008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175363
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the steady states of the spherically symmetric Einstein-Vlasov system
dc.typetext

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