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Entropy of black holes with arbitrary shapes in loop quantum gravity 被引量:1
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作者 ShuPeng Song haida li +1 位作者 YongGe Ma Cong Zhang 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2021年第12期76-83,共8页
The quasi-local notion of an isolated horizon is employed to study the entropy of black holes without any particular symmetry in loop quantum gravity. The idea of characterizing the shape of a horizon by a sequence of... The quasi-local notion of an isolated horizon is employed to study the entropy of black holes without any particular symmetry in loop quantum gravity. The idea of characterizing the shape of a horizon by a sequence of local areas is successfully applied in the scheme to calculate the entropy by the S O(1, 1) BF boundary theory matching loop quantum gravity in the bulk. The generating function for calculating the microscopical degrees of freedom of a given isolated horizon is obtained. Numerical computations of small black holes indicate a new entropy formula containing the quantum correction related to the partition of the horizon. Further evidence shows that, for a given horizon area, the entropy decreases as a black hole deviates from the spherically symmetric one,and the entropy formula is also well suitable for big black holes. 展开更多
关键词 isolated horizon ENTROPY loop quantum gravity
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