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Symmetric and asymmetric nuclear matter in the Thomas-Fermi model at finite temperatures

Klaus Strobel·Fridolin Weber·Manfred K. Weigel
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Abstract

The properties of warm symmetric and asymmetric nuclear matter are investigated in the frame of the Thomas-Fermi approximation using a recent modern parametrization of the effective nucleon-nucleon interaction of Myers and Swiatecki. Special attention is paid to the liquid-gas phase transition, which is of special interest in modern nuclear physics. We have determined the critical temperature, critical density and the so-called flash temperature. Furthermore the equation of state for cold neutron star matter was calculated.

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Klaus Strobel, Fridolin Weber, Manfred K. Weigel. 1998-10-01. Symmetric and asymmetric nuclear matter in the Thomas-Fermi model at finite temperatures. https://doi.org/10.1515/zna-1999-0111

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