Kinetic theory in astrophysics and cosmology

Astronomy and Astrophysics – Astrophysics

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Distribution Functions, Einstein Equations, Galaxies, Kinetic Theory, Maxwell-Boltzmann Density Function, Star Clusters, Astrophysics, Charged Particles, Cosmology, Hydrodynamics, Relativistic Theory

Scientific paper

Ehler's (1971) Killing vector approach of kinetic theory is generalized to include charged particles. This approach is first applied to static spherically symmetric models, and a static distribution of charged particles is obtained where the electrical repulsion is balanced by the gravitational attraction. The Killing vector approach is then applied to the G4 VIII space-time, and it is concluded that this space-time cannot be generated by a perfect fluid in kinetic theory. These results call into question the physical meaning of perfect-fluid solutions in such space-times; presumably many of the Bianchi models would share this difficulty. It is not possible for the G4 VIII space-time to be generated by charged matter. This implies that the source-free magnetic fields present in exact solutions for this model must arise from an earlier, more chaotic state of the universe, or be given as initial conditions.

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