| Abstract: |
| In nonlinear PDE theories, there are several description of gaseous stars, depending on their scopes and equation of states. In microscopic scale, quantum mechanical descriptions of stars are given by Hartree or Hartree-Fock equations while the Euler-Poisson equations replace this in macroscopic scale. In this talk, we discuss about the existence, properties such as shape or stability of these stars and interconnection between them. |
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