What is the time dependence of the evolution of the observed ratio of dark energy to baryonic matter? The density-of-the-universe ratio varies from about (zero):1 at approximately 380,000 years after the big bang to about (15 to 18):1 at approximately today. [I infer the latter number from J. Beringer et al. (Particle Data Group), Phys. Rev. D86, 010001 (2012); http://pdg.lbl.gov/2012/reviews/rpp2012-rev-astrophysical-constants.pdf.] Have analyses estimated the evolution of the ratio, between the two times? Can someone point me to such results? Do any theories predict such results?