A COMPUTATION OF THE EQUATION OF STATE FOR A FERMI GAS
Articles > Article · 1992
Authors: Mutlu YILDIZ, DİLHAN ERYURTEZER
ASTROPHYSICS AND SPACE SCIENCE, Journal Indexed in SCI Expanded, International, 1992, vol 190, pp 233-242
DOI: 10.1007/bf00644850
Summary
Calculation of equation of state in stellar interiors becomes difficult as contained gas deviates from perfect gas. We present a method for the calculation of electron pressure in terms of density and temperature in the presence of degeneracy. The method is applicable for T < 10(9) K, and requires complete ionization.