arXiv · hep-th/0211096
The Rotating Quantum Thermal Distribution
Abstract
We show that the rigidly rotating quantum thermal distribution on flat space-time suffers from a global pathology which can be cured by introducing a cylindrical mirror if and only if it has a radius smaller than that of the speed-of-light cylinder. When this condition is met, we demonstrate numerically that the renormalized expectation value of the energy-momentum stress tensor corresponds to a rigidly rotating thermal bath up to a finite correction except on the mirror where there are the usual Casimir divergences.
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Gavin Duffy, Adrian C. Ottewill. 2002-11-11. The Rotating Quantum Thermal Distribution. https://doi.org/10.1103/physrevd.67.044002
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