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Temperature evolution of thermodynamic functions from symmetric to asymmetric nuclear matter

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This paper investigates thermal properties of nuclear matter using the Friedman-Pandharipande- Ravenhall equation of state. Thermodynamic quantities such as internal energy, entropy and free energy are calculated both for symmetric and asymmetric nuclear matter for temperatures ranging up to 30 MeV. A change of free energy curvature indicates the liquid-gas phase transition in nuclear matter.
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online
2015-04-09
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bwmeta1.element.ojs-nameId-6e3e8ea9-5a94-37a7-828b-e6cd5da23db6-year-2015-article-1603
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