Self-gravitating stationary spherically symmetric systems in relativistic galactic dynamics

DOI10.1017/S0305004107000540zbMath1233.85003arXivgr-qc/0609074OpenAlexW3106092747MaRDI QIDQ5434694

J. Mark Heinzle, Claes Uggla, Mikael Fjällborg

Publication date: 7 January 2008

Published in: Mathematical Proceedings of the Cambridge Philosophical Society (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0609074

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Vlasov equations (35Q83) PDEs in connection with astronomy and astrophysics (35Q85)

Related Items

Cosmological global dynamical systems analysis ⋮ Bianchi cosmologies with anisotropic matter: locally rotationally symmetric models ⋮ Existence of axially symmetric static solutions of the Einstein-Vlasov system ⋮ A variational approach to relativistic fluid balls ⋮ Asymptotics of LRS Bianchi type I cosmological models with elastic matter ⋮ The Einstein-Vlasov system/kinetic theory ⋮ Asymptotic behavior and orbital stability of galactic dynamics in relativistic scalar gravity

Cites Work

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• Existence and properties of spherically symmetric static fluid bodies with a given equation of state
• Theory of Newtonian self-gravitating stationary spherically symmetric systems
• Dynamical systems approach to relativistic spherically symmetric static perfect fluid models
• Asymptotic states of magnetic Bianchi VI cosmologies
• Compact support of spherically symmetric equilibria in non-relativistic and relativistic galactic dynamics