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  • Access by Xinjiang University

Pressure and composition of a weakly degenerate nucleon gas

Russell W. Evans* and Peter B. Shaw

  • Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802

  • *Present address: Lincoln Laboratories, MIT, Lexington, Massachusetts 02173.

Phys. Rev. D 14, 2526 – Published 15 November, 1976

DOI: https://doi.org/10.1103/PhysRevD.14.2526

Abstract

The equation of state and species concentrations of a hot neutral gas of neutrons, protons, electrons, positrons, and muons are determined in the temperature range 5×1010-5×1011°K and density range 5×1010-1014 g/cm3. The gas is considered to be in local thermal and chemical equilibrium under the effect of weak and strong interactions. A virial expansion is constructed to include second-order statistical and dynamical terms, the latter through experimental nucleon-nucleon scattering phase shifts. Decreases in pressure and increases in electron number densities are found to be quite modest.

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