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Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence

James V. Lindesay·H. Pierre Noyes
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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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James V. Lindesay, H. Pierre Noyes. 2004-10-25. Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence. https://arxiv.org/abs/astro-ph/0410217

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