Cosmic Microwave Background Fluctuation Amplitude from Dark Energy De-Coherence
نویسنده
چکیده
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. PACS numbers: 98.80.Bp, 98.80.Jk, 95.30.Sf
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