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 towards the weak coupling regime driven by the exponential dilaton potential. It also holds in other simple cases.
|頁（從 - 到）||3281-3292|
|期刊||Classical and Quantum Gravity|
|出版狀態||已發佈 - 2002 6月 21|
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