The Finite Temperature Nucleon Matter. I : The Case of Neutron Gas

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概要

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• Equations of state of pure neutron gas at finite temperature is investigated with the aid of the extended method of the Brueckner theory (the low temperature case) and the virial expansion method ( the high temperature case). Computations are worked out for the regions of the temperature 1 MeV<T<50 MeV and the density 10^<12.5> g/cm^3<ρ<10^<14.5> g/cm^3, in which regions imploding supernova cores run. By this overall examination from the low to high temperature the behavior of the equation of state of the high density matter is made clear. As a result, it is found that there exists an approximate equation of state adequate for practical uses.

• 理論物理学刊行会の論文
• 1977-05-25

著者

• Kiguchi Masayoshi

  Department Of Physics Kyoto University

関連論文

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• The Quantum Chromodynamic Black Body Radiation and the Universe
• Neutrino Cooling of Neutron Stars by Percolating Quarks
• The Finite Temperature Nucleon Matter. I : The Case of Neutron Gas

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