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So far we have considered highly dilute (ideal) gases in which the interaction between the particles could be neglected. In the following we will consider moderately diluted and interacting gases; for the sake of simplicity we consider gas particles without spin, i.e. \((2s+1) = 1\) . As important example we will investigate the properties of a classical Van der Waals gas as well as ‘nuclear matter’ in thermal equilibrium as an example for an interacting Fermi system.

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Real Interacting Gases

  • 章节

  • 发表日期：

    2025年

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  • Wolfgang Cassing

摘要

So far we have considered highly dilute (ideal) gases in which the interaction between the particles could be neglected. In the following we will consider moderately diluted and interacting gases; for the sake of simplicity we consider gas particles without spin, i.e. \((2s+1) = 1\) . As important example we will investigate the properties of a classical Van der Waals gas as well as ‘nuclear matter’ in thermal equilibrium as an example for an interacting Fermi system.