Christian L Reichardt, Roland de Putter, Oliver Zahn, Zhen Hou
We present new limits on early dark energy from the cosmic microwave
background (CMB) using data from the WMAP satellite on large angular scales and
South Pole Telescope (SPT) on small angular scales. We find a strong upper
limit on the early dark energy density of Omega_e < 0.018 at 95% confidence, a
factor of three improvement over WMAP data alone. We show that adding
lower-redshift probes of the expansion rate to the CMB data improves
constraints on the dark energy equation of state, but not the early dark energy
density. We also explain how the small-scale CMB temperature anisotropy
constrains early dark energy.
View original:
http://arxiv.org/abs/1110.5328
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