Theory of Newtonian self-gravitating stationary spherically symmetric systems

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dc.creatorHeinzle, J. Mark
dc.creatorRendall, Alan D.
dc.creatorUggla, Claes
dc.date2004-08-25
dc.date.accessioned2026-07-07T08:39:33Z
dc.date.available2026-07-07T08:39:33Z
dc.descriptionWe investigate spherically symmetric equilibrium states of the Vlasov-Poisson system, relevant in galactic dynamics. We recast the equations into a regular three-dimensional system of autonomous first order ordinary differential equations on a region with compact closure.Based on a dynamical systems analysis we derive theorems that guarantee that the steady state solutions have finite mass and compact support.
dc.description18 pages; 4 figures
dc.identifierhttps://arxiv.org/abs/math-ph/0408045
dc.identifierhttp://arxiv.org/abs/math-ph/0408045
dc.identifierMath. Proc. Camb. Phil. Soc. 140: 177-192, 2006.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141108
dc.subjectMathematical Physics
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subject37Cxx; 85A05
dc.titleTheory of Newtonian self-gravitating stationary spherically symmetric systems
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