Chaos in Galaxies
نویسنده
چکیده
1. Like in 3D hydrodynamics, the non-linearity of the Poisson-Boltzmann system may imply dissipation through the growth of discontinuous solutions. 2. The relationship between the microscopic exponential sensitivity of N-body systems and the stability of mean field galaxy models. 3. The role of quantum physics in the dynamics of structure formation, considering that cosmological neutrinos are massive and semi-degenerate fermions.
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تاریخ انتشار 2008