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Note on holographic RG flow in string cosmology
2002
Classical and quantum gravity
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
doi:10.1088/0264-9381/19/12/311
fatcat:5f2vjrkpyja7lbjbr6ncyn36c4