arXiv · hep-th/9411130
High-temperature QCD and the classical Boltzmann equation in curved spacetime
Abstract
It has been shown that the high-temperature limit of perturbative thermal QCD is easily obtained from the Boltzmann transport equation for `classical' coloured particles. We generalize this treatment to curved space-time. We are thus able to construct the effective stress-energy tensor. We give a construction for an effective action. As an example of the convenience of the Boltzmann method, we derive the high-temperature 3-graviton function. We discuss the static case.
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F. T. Brandt, J. Frenkel, J. C. Taylor. 1994-11-17. High-temperature QCD and the classical Boltzmann equation in curved spacetime. https://doi.org/10.1016/0550-3213(94)00582-y
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