Abstract
The coincidence problem of late cosmic acceleration constitutes a serious riddle with regard to our understanding of the evolution of the Universe. Here we argue that this problem may someday be solved-or better understood-by expressing the Hubble expansion rate as a function of the ratio of densities (dark matter/dark energy) and observationally determining the said rate in terms of the redshift.
Original language | English |
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Article number | 021302 |
Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volume | 78 |
Issue number | 2 |
DOIs | |
State | Published - 14 Jul 2008 |