arXiv · hep-th/9604054
Computation of the winding number diffusion rate due to the cosmological sphaleron
Abstract
A detailed quantitative analysis of the transition process mediated by a sphaleron type non-Abelian gauge field configuration in a static Einstein universe is carried out. By examining spectra of the fluctuation operators and applying the zeta function regularization scheme, a closed analytical expression for the transition rate at the one-loop level is derived. This is a unique example of an exact solution for a sphaleron model in $3+1$ spacetime dimensions.
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Mikhail S. Volkov. 1996-07-23. Computation of the winding number diffusion rate due to the cosmological sphaleron. https://doi.org/10.1103/physrevd.54.5014
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