在Horava-Lifshitz引力下类Schwarzschild黑洞的熵

Entropy of the Similar Schwarzschild Black Hole in the Deformed Horava-Lifshitz Gravity

在薄层模型brick-wall方法的基础上,进一步研究了在Horava-Lifshitz引力下类Schwarzschild黑洞的熵,发现仍然与视界面积成正比,并且对每一个局部也是成立的.这表明引力的修正不会改变黑洞的热力学特性.

On the basis of thin film brick-wall method,entropy of the similar Schwarzschild black hole in the deformed Horava-Lifshitz gravity is studied deeply.It is found that the entropy still is proportional to the area of the visible horizon,and on the every cell on the event visible horizon is also true.This shows that the gravity of the amendment will not change the thermodynamic properties of black holes