Entropy Bounds and Dark Energy
arXiv:hep-th/0403052 · doi:10.1016/j.physletb.2004.05.020
Abstract
Entropy bounds render quantum corrections to the cosmological constant finite. Under certain assumptions, the natural value of is of order the observed dark energy density , thereby resolving the cosmological constant problem. We note that the dark energy equation of state in these scenarios is over cosmological distances, and is strongly disfavored by observational data. Alternatively, in these scenarios might account for the diffuse dark matter component of the cosmological energy density.
6 pages, Latex. Added discussion of non-cosmological limits on holographic dark energy. Version to appear in Physics Letters B
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