We examine conditions for which energy flows in the early universe are modeled as a quantum Hamilton-Jacobi set of equations. Subsequently, we manage to use the Heisenberg Uncertainty principle for metric tensors based upon are Geometrodynamics treatment of our problem
Comments: 16 Pages. Last version of a paper cleared by referees in the Ukranian Journal of Physics. Subsequently accepted for Publication, after 1 year of vetting
[v1] 2017-01-15 00:36:12
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