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Black Hole Thermodynamics of Hořava-Lifshitz and IR Modified Ho řava-Lifshitz Gravity Theory

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Abstract

Recently, a renormalizable model of gravity has been proposed by Hoř ava, which might be an ultraviolet completion of general relativity and it reduces to Einstein gravity with a non-vanishing cosmological constant in infrared approximation. Kehagias and Sfetsos have added a relevant operator proportional to the 3D geometry Ricci scalar to the original Hoř ava-Lifshitz theory action, which “softly” deviated from detailed-balance. This does not modify the ultraviolet properties of the theory. However, it modifies the infrared approximation and the Minkowski vacuum can be allowed in the infrared Hořava-Lifshitz gravity theory. The static spherical symmetric black hole solutions have been obtained in the Hořava-Lifshitz and infrared Hořava-Lifshitz gravity theory. Based on the metric of the black holes, Hawking radiation of massless scalar particles is investigated using Damour-Ruffini method. Then the black hole thermodynamics property will also be discussed.

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  1. Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing, 100875, China

    Shi-Wei Zhou & Wen-Biao Liu

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  1. Shi-Wei Zhou
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  2. Wen-Biao Liu
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Correspondence to Wen-Biao Liu.

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Zhou, SW., Liu, WB. Black Hole Thermodynamics of Hořava-Lifshitz and IR Modified Ho řava-Lifshitz Gravity Theory. Int J Theor Phys 50, 1776–1784 (2011). https://doi.org/10.1007/s10773-011-0686-1

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  • DOI: https://doi.org/10.1007/s10773-011-0686-1

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