What is it about?
Many of the properties of nuclear systems are similar to those of gases. In this article we use classical Newtonian mechanics to study nuclear liquid and gaseous phases, and properties such as phase information, the Maxwell construction, spinodal lines and symmetry energy.
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Why is it important?
Large nuclear systems exist in, for instance, neutron stars, and their properties -such as its cooling- depend on the thermodynamics of such large systems.
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This page is a summary of: Thermodynamics of neutron-rich nuclear matter, January 2016, American Institute of Physics,
DOI: 10.1063/1.4955359.
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