Dark Energy Without Dark Energy:. Average Observational Quantities

Details Dark Energy Without Dark Energy:. Average Observational Quantities Dark Energy Without Dark Energy:. Average Observational Quantities

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dmap.conf..397w&link_type=abstract

DARK MATTER IN ASTROPHYSICS AND PARTICLE PHYSICS . Proceedings of the 7th International Heidelberg Conference on Dark 2009 . Hel

Astronomy and Astrophysics

Astrophysics

Dark Energy, Theoretical Cosmology, Observational Cosmology

Scientific paper

I discuss potential observational tests of a "radically conservative" solution to the problem of dark energy in cosmology, in which the apparent acceleration of the universe is understood as a consequence of gravitational energy gradients that grow when spatial curvature gradients become significant with the nonlinear growth of cosmic structure. In particular, I discuss measures equivalent to the dark energy equation of state, baryon acoustic oscillation statistic DV, H(z), the Om(z) diagnostic, an average inhomogeneity diagnostic, and the time-drift of cosmological redshifts.

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