York / Suntzeff / Yanny / Odintsov / B. / Nunes / London / /
Country
Australia / / /
Facility
University of New South Wales / Australian National University / /
IndustryTerm
dark matter-dark energy interaction / e-prints / gas models / non-canonical kinetic energy / energy component / dark energy densities / dark energy model / dark-energy-matter unification / quintessence energy decays / energy constraints / satisfactory solution / pure vacuum energy / kinetic energy / dark energy / dark energy dynamics / tracker solution / vacuum energy wde / stable tracker solution / Online Archive / chaplygin gas models / energy densities / vacuum energy / vacuum energy density / dark energy density / energy density / typical k-essence energy density history / dark energy component / cosmic energy density history / Dark energy candidates / exotic dark energy models / phantom energy / quintessence energy / energy density history / field energy decays / attractor solutions / e-folds / planetary systems / quintessence energy density / dark energy models / dark energy equation / observed dark energy density / energy / /
ProvinceOrState
South Dakota / New Jersey / New Brunswick / Copeland / Delaware / New South Wales / /
PublishedMedium
Astronomy and Astrophysics / Classical and Quantum Gravity / Physical Review Letters / /
Draft version July 30, 2007 Preprint typeset using LATEX style emulateapj v[removed]DARK-ENERGY DYNAMICS REQUIRED TO SOLVE THE COSMIC COINCIDENCE Chas A. Egan1,2 & Charles H. Lineweaver2 Draft version July 30, 2007