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    <pubDate>Mon, 05 May 2008 07:54:37 +0200</pubDate>
    <lastBuildDate>Mon, 05 May 2008 07:54:37 +0200</lastBuildDate>
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      <title>Existence and stability of stellardynamic models</title>
      <link>http://opus4.kobv.de/opus4-ubbayreuth/frontdoor/index/index/docId/383</link>
      <description>We examine existence and stability of stationary solutions to the Vlasov-Poisson system. This system is used in stellardynmaics to describe the evolution of galaxies where collissions are neglected and the evolution is determined by the self-consistent gravitational field which is created by the particles, e.g. the stars . In the first part we examine steady states which decsribe static shells under the influence of a fixed point mass. These solutions can be used as a model for a galaxy with a massive black hole in its center. For the Vlasov--Poisson system under the influence of such a point mass, we prove a global existence result. In the second part, we construct axially symmetric solutions depending on Jacobis integral. The presented results are in accordance with the numerical examinations of the P.O. Vandervoort.</description>
      <author>Achim Schulze</author>
      <category>doctoralthesis</category>
      <guid>http://opus4.kobv.de/opus4-ubbayreuth/frontdoor/index/index/docId/383</guid>
      <pubDate>Mon, 05 May 2008 07:54:37 +0200</pubDate>
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