Physics – Plasma Physics
Scientific paper
Jan 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..221g&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 1, Jan. 1983, p. 221-228.
Physics
Plasma Physics
1
Cosmic Plasma, Degenerate Matter, Dense Plasmas, Equations Of State, Plasma Physics, Hadrons, Pressure Gradients, Relativistic Plasmas, Stellar Models, Thermodynamics
Scientific paper
The importance of eliminating any inaccuracies in the equation of state is emphasized. It is noted that with the progress made in elementary particle physics, it has become possible to derive, more or less precisely, an equation of state of degenerate stellar matter in relativistic objects. The study presented here is a continuation of the work reported by Sahakian and Grigorian (1977, 1979, 1980). In those studies, the thermodynamic properties of degenerate plasma were investigated, and approximations were obtained for the state equation rho(P) under conditions where it was impossible to derive any analytical dependence. Even though these approximate formulas are useful for determining the parameters of degenerate configurations, they prove to be unsatisfactory for solving certain other special problems, such as the configuration stability or the elastic wave propagation velocity in the plasma. On the basis of general requirements, the parameters of the hadronic plasma and the state equation of degenerate superdense matter in the entire range of pressures are improved and corrected.
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