CMB Fluctuation Amplitude from Dark Energy Partitions
arXiv:astro-ph/0412477 · doi:10.1016/j.physletb.2005.12.026
Abstract
It is assumed that the dark energy observed today is frozen as a result of a phase transition involving the source of that energy. Postulating that the dark energy de-coherence which results from this phase transition drives statistical variations in the energy density specifies a class of cosmological models in which the cosmic microwave background (CMB) fluctuation amplitude at last scattering is approximately .
7 Pages, Poster presented at Texas@Stanford conference, Dec. 2004, minor clarifications