Investigation of the equation of state of astrophysical bodies by the LMTO method

Details Investigation of the equation of state of astrophysical bodies by the LMTO method Investigation of the equation of state of astrophysical bodies by the LMTO method

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...242..510g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 242, no. 2, Feb. 1991, p. 510-512.

Statistics

Computation

Celestial Bodies, Computational Astrophysics, Equations Of State, Stellar Evolution, White Dwarf Stars, Distribution Functions, Fermi Surfaces, Helium, Hydrogen, Linear Equations

Scientific paper

The electronic contribution to the equation of state at high densities and low temperatures was calculated using two basically different methods: the first method is based on electronic plane waves while the second is based on lattice electronic wave functions. The purpose of the comparison is to determine the accuracy of the equation of state that is normally used in stellar evolution calculations (which is based on plane waves) in the region of pressure ionization.

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