CMB Fluctuation Amplitude from Dark Energy Partitions

Details CMB Fluctuation Amplitude from Dark Energy Partitions CMB Fluctuation Amplitude from Dark Energy Partitions

2004-12-17

arxiv.org/abs/astro-ph/0412477v3

Phys.Lett. B633 (2006) 433-435

Astronomy and Astrophysics

Astrophysics

7 Pages, Poster presented at Texas@Stanford conference, Dec. 2004, minor clarifications

Scientific paper

10.1016/j.physletb.2005.12.026

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 $10^{-5}$.

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