Equilibrium Configurations of Self-Gravitating Non-Collisional Systems with a Phase-Space Cut-Off

Details Equilibrium Configurations of Self-Gravitating Non-Collisional Systems with a Phase-Space Cut-Off Equilibrium Configurations of Self-Gravitating Non-Collisional Systems with a Phase-Space Cut-Off

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.1647m&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

We extend the gravitational Fermi gas model approach to the case of finite temperature, following the same scheme as the T = 0K case: writing the Poisson equation for the Newtonian gravity case and the Oppenheimer-Volkoff equations for the general relativistic case. The role of the Fermi energy is played by an energy cut-off Ec, the distribution functions used are the nondegenerate Fermi-Dirac one and the Maxwell-Boltzmann one, both truncated by Ec.

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