Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence

Details Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence

2004-10-07

arxiv.org/abs/astro-ph/0410217v2

Astronomy and Astrophysics

Astrophysics

9 pages, 1 figure

Scientific paper

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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