MODELLING THE CORE AND THE HALO OF GALAXIES BY FERMIONS

Andrea GeralicoPhysics Department and ICRA, University of Rome "La Sapienza," I-00185 Rome, ItalyR. RuffiniPhysics Department and ICRA, University of Rome "La Sapienza," I-00185 Rome, Italy

2012en

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Annotatsiya

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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DOI: 10.1142/s2010194512006368

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