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Über Familien sphärisch symmetrischer stationärer Lösungen des ...

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ABSTRACT<br />

The present thesis is concerned with an investigation of families of steady states<br />

of the Vlasov-Poisson system. This nonlinear system of partial differential equations<br />

can be used for the dynamical <strong>des</strong>cription of a closed large particle ensemble<br />

in a six-dimensional phase space, only interacting by gravity.<br />

For the construction of stationary solutions we use a well-known approach<br />

by making an ansatz for the density on phase space as a function of the particle<br />

energy. According to a more general result of Gidas, Ni and Nirenberg<br />

[7] solutions of this type are always spherically symmetric, whereby the angular<br />

momentum is conserved along solutions of the characteristic system of<br />

the Vlasov equation. Therefore, up to technical details, any function of these<br />

conserved quantities satisfies the Vlasov equation, and it remains to solve a<br />

semilinear Poisson equation which, due to spherical symmetry, reduces to a<br />

second-order integro-differential equation. Several papers in recent years have<br />

adressed the question under which assumptions on the ansatz function related<br />

solutions have finite mass and compact support (cf. Rein and Rendall [20]<br />

or Heinzle, Rendall and Ugla [8]).<br />

For the outlined approach we give a new and simple proof for the compactness<br />

of the support of the resulting solutions. Our method easily applies to a whole<br />

class of systems (Vlasov-Poisson, relativistic Vlasov-Poisson, Einstein-Vlasov,<br />

Euler-Poisson and Einstein-Euler system) so that they can unlike before be<br />

treated by the same method. Moreover, the conditions we give are slight generalizations<br />

to such conditions known.<br />

In general, the set of steady states related to an ansatz function can in a<br />

natural way be seen as one-parameter family. The qualitative structure of the<br />

iii

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