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astro-ph2000
Thermodynamical properties of stellar matter: II. Internal energy, temperature and density exponents and specific heats for stellar interiors
W. Stolzmann, T. Bloecker
Starting from the Helmholtz free energy we calculate analytically first- and second-order derivatives, as internal energy and specific heats, for the ideal system and the exchange…
astro-ph1998★ 2 cited
A Semi-relativistic Equation of State for Stellar Interiors
W. Stolzmann, T. Bloecker
Using the technique of Pade Approximants for the correlation contributions of charged particles we are able to reproduce complex mathematical expressions by simple algebraic formul…