dorsal/arxiv
View SchemaSymmetric and asymmetric nuclear matter in the Thomas-Fermi model at finite temperatures
| Authors | Klaus Strobel, Fridolin Weber, Manfred K. Weigel |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9810003 |
| URL | https://arxiv.org/abs/nucl-th/9810003 |
| DOI | 10.1515/zna-1999-0111 |
| Journal | Z. Naturforsch. 54a (1999) 83-90 |
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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"abstract": "The properties of warm symmetric and asymmetric nuclear matter are\ninvestigated in the frame of the Thomas-Fermi approximation using a recent\nmodern parametrization of the effective nucleon-nucleon interaction of Myers\nand Swiatecki. Special attention is paid to the liquid-gas phase transition,\nwhich is of special interest in modern nuclear physics. We have determined the\ncritical temperature, critical density and the so-called flash temperature.\nFurthermore the equation of state for cold neutron star matter was calculated.",
"arxiv_id": "nucl-th/9810003",
"authors": [
"Klaus Strobel",
"Fridolin Weber",
"Manfred K. Weigel"
],
"categories": [
"nucl-th",
"astro-ph"
],
"doi": "10.1515/zna-1999-0111",
"journal_ref": "Z. Naturforsch. 54a (1999) 83-90",
"title": "Symmetric and asymmetric nuclear matter in the Thomas-Fermi model at finite temperatures",
"url": "https://arxiv.org/abs/nucl-th/9810003"
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