Symmetric and asymmetric nuclear matter in the Thomas-Fermi model at finite temperatures
arXiv:nucl-th/9810003 · doi:10.1515/zna-1999-0111
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.
20 pages, 12 figures, to be published in Z. Naturforsch. A