arXiv · hep-th/0111201
Note on Holographic RG Flow in String Cosmology
Abstract
We propose a new holographic C-function for the accelerating universe defined in the stringy frame motivated mainly by the fact that the number of degrees of freedom should be infinite for a physical system of infinite size. This is the generalization of Strominger's recent proposal of the holographic C-function to the asymptotically non-de Sitter universe. We find that the corresponding C-theorem holds true if the universe accelerates toward the weak coupling regime driven by the exponential dilaton potential. It also holds in other simple cases.
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Miao Li, Feng-Li Lin. 2002-05-08. Note on Holographic RG Flow in String Cosmology. https://doi.org/10.1088/0264-9381%2F19%2F12%2F311
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