MODELLING THE CORE AND THE HALO OF GALAXIES BY FERMIONS
Andrea GeralicoPhysics Department and ICRA, University of Rome "La Sapienza," I-00185 Rome, ItalyR. RuffiniICRANet, I-65100 Pescara, Italy
2012en
ABI
Abstract
The possibility to describe in a consistent way both the supermassive compact object at the center and the halo of galaxies is explored by assuming the existence of a self-gravitating semi-degenerate system of fermions in thermodynamical equilibrium.
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Cited by 10 references