Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence
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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 $10^{-5}$.
9 pages, 1 figure
9 pages, 1 figure