A new statistical mechanical formalism for gases
R. D. Rohrmann

TL;DR
This paper introduces a novel statistical mechanical formalism for gases that unifies thermodynamics and microstructure analysis, with applications to astrophysical atmospheres and ionized hydrogen gases.
Contribution
It develops a new equilibrium theory based on space distribution among particles, providing both thermodynamic and structural insights in a unified framework.
Findings
Derived equations of state and distribution functions in multiple dimensions.
Applied formalism to describe atomic populations in ionized hydrogen gas.
Enabled detailed evaluation of atomic density and internal states.
Abstract
An equilibrium theory of classical fluids based on the space distribution among the particles is derived in the framework of the energy minimization method. This study is motivated by current difficulties of evaluation of optical properties in atmospheres of degenerate stars. Present paper focuses on diluted one-component systems, where the interaction energy is calculated as a sum of binary contributions. The spatial configuration of the gas is described in terms of a particle-state variable v which roughly measures the free space surrounding each particle. The formalism offers a unified treatment of both thermodynamics and structure of fluids, since it not only provides the state function (the Helmholtz free energy) of a fluid, but also automatically gives information on the microstructure of the system (e.g. the nearest-neighbor distribution function). Equations of state and…
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