Remarks on the evaluation of critical parameters in self-gravitating systems

Details Remarks on the evaluation of critical parameters in self-gravitating systems Remarks on the evaluation of critical parameters in self-gravitating systems

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..82..241b&link_type=abstract

Astrophysics and Space Science, vol. 82, no. 1, Feb. 1982, p. 241-246.

Astronomy and Astrophysics

Astrophysics

Fermions, Main Sequence Stars, Stellar Gravitation, Stellar Models, Thermodynamics, Astrophysics, B Stars, Free Energy, Gas Pressure, Radii, Stellar Evolution, Stellar Temperature

Scientific paper

The Thirring (1972) model is used in an investigation of the thermodynamic qualities of a system of self-gravitating fermions, where expressions for the free energy and pressure of the gravitating system are applied to a star. The critical radius and temperature values derived indicate the existence of a transition after the Main Sequence stage, marked by the onset of a core-halo structure.

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