The Friedmann equations in deformed Hořava-Lifshitz gravity and Debye model
arXiv:1007.2985 · doi:10.1142/S0218271811018585
Abstract
Considering the results from Hořava-Lifshitz (HL) theory, a more precise relation between the number of bits and area in the holographic system is proposed. With this corrected relation and Debye model, two modified Friedmann equations are derived from the Hawking temperature and the Unruh temperature separately in entropic force. These equations could be better in describing the whole evolution of the universe.
arXiv commentSome typos are corrected, and new references added. Version to appear in International Journal of Modern Physics D
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