Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence
James V. Lindesay, H. Pierre Noyes
Abstract
Standard cosmology connects the scale generated at late times by the cosmological constant with that generated in early times by the energy dynamics. Assuming dark energy de-coherence occurs during early times when the scale parameter expansion rate is no longer supra-luminal specifies a class of cosmological models in which the cosmic microwave background fluctuation amplitude at last scattering is approximately 10-5.
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