A computation of the equation of state for a Fermi gas

Details A computation of the equation of state for a Fermi gas A computation of the equation of state for a Fermi gas

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.190..233y&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 190, no. 2, April 1992, p. 233-242.

Statistics

Computation

1

Computational Astrophysics, Electron Gas, Equations Of State, Stellar Interiors, Electron Density (Concentration), Electron Pressure, Ideal Gas, Stellar Models

Scientific paper

A method for calculating the electron pressure for a Fermi gas is developed, making it possible to calculate the equation of state in stellar interiors. The method is applicable for temperatures below 10 exp 9 K, this upper limit being selected in order to be able to avoid the processes such as inverse beta-decay and the electron-positron pair formation. The method is applied to calculations of stellar density, temperature, and chemical compositions at the center of low mass stars, with the results presented in tabular form.

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