Temperature in relativistic fluids
arXiv:2210.15605 · doi:10.1103/PhysRevD.107.086012
Abstract
For static matter in a gravitational field, different conventions for equilibrium local temperature exist in the classic physics literature. We illustrate the difference between two popular conventions using black-body radiation in a spherically symmetric gravitational potential. Equilibrium temperatures defined by the "Landau frame" or "Eckart frame" prescriptions most commonly used in relativistic fluid dynamics do not satisfy the statistical-mechanical relation .
arXiv comment14 pages, 3 figures. V2: Small clarifications, version accepted for publication in PRD
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