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Statistical mechanics and phase diagrams of rotating self-gravitating fermions
ASTRONOMY & ASTROPHYSICS, no. 1 (2003): 1-17
Abstract
We compute statistical equilibrium states of rotating self-gravitating fermions by maximizing the Fermi-Dirac entropy at fixed mass, energy and angular momentum. We describe the phase transition from a gaseous phase to a condensed phase ( corresponding to white dwarfs, neutron stars or fermion balls in dark matter models) as we vary energ...More
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