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Corrections to entropy and thermodynamics of charged black hole using generalized uncertainty principle

机译:用带电荷校正带电黑洞的熵和热力学   广义不确定性原理

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摘要

Recently, there has been much attention devoted to resolving the quantumcorrections to the Bekenstein-Hawking (black hole) entropy, which relates theentropy to the cross-sectional area of the black hole horizon. Usinggeneralized uncertainty principle (GUP), corrections to the geometric entropyand thermodynamics of black hole will be introduced. The impact of GUP on theentropy near the horizon of three types of black holes; Schwarzschild,Garfinkle-Horowitz-Strominger and Reissner-Nordstr\"om is determined. It isfound that the logarithmic divergence in the entropy-area relation turns to bepositive. The entropy $S$, which is assumed to be related to horizon'stwo-dimensional area, gets an additional terms, for instance $2\, \sqrt{\pi}\,\alpha\, \sqrt{S}$, where $\alpha$ is the GUP parameter.
机译:近来,已经有很多注意力致力于解决对Bekenstein-Hawking(黑洞)熵的量子校正,该量子校正将熵与黑洞视界的横截面积相关联。利用广义不确定性原理(GUP),将对黑洞的几何熵和热力学进行校正。 GUP对三种类型黑洞地平线附近熵的影响;确定了Schwarzschild,Garfinkle-Horowitz-Strominger和Reissner-Nordstr \“ om。发现熵-面积关系的对数散度变为正。尺寸区域,则获得其他条件,例如$ 2 \,\ sqrt {\ pi} \,\ alpha \,\ sqrt {S} $,其中$ \ alpha $是GUP参数。

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