arXiv · 1910.06791
Relativistic kinematic approach to the classical ideal gas
Abstract
he necessary and sufficient conditions for a unit time-like vector field to be the unit velocity of a classical ideal gas are obtained. In a recent paper [Coll, Ferrando and S\'aez, Phys. Rev D {\bf 99} (2019)] we have offered a purely hydrodynamic description of a classical ideal gas. Here we take one more step in reducing the number of variables necessary to characterize these media by showing that a plainly kinematic description can be obtained. We apply the results to obtain test solutions to the hydrodynamic equation that model the evolution in local thermal equilibrium of a classical ideal gas. \end{abstract}
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Joan Josep Ferrando, Juan Antonio Sáez. 2019-10-15. Relativistic kinematic approach to the classical ideal gas. https://doi.org/10.1088/1361-6382%2Fab4229
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