Horizon thermodynamics in f(R,R^μνRμν)theory  

作　　者：Haiyuan Feng Rong-Jia Yang 冯海源;杨荣佳(College of Physical Science and Technology,Hebei University,Baoding 071002,China;Hebei Key Lab of Optic-Electronic Information and Materials,Hebei University,Baoding 071002,China;National-Local Joint Engineering Laboratory of New Energy Photoelectric Devices,Hebei University,Baoding 071002,China;Key Laboratory of High-pricision Computation and Application of Quantum Field Theory of Hebei Province,Hebei University,Baoding 071002,China)

机构地区：[1]College of Physical Science and Technology,Hebei University,Baoding 071002,China [2]Hebei Key Lab of Optic-Electronic Information and Materials,Hebei University,Baoding 071002,China [3]National-Local Joint Engineering Laboratory of New Energy Photoelectric Devices,Hebei University,Baoding 071002,China [4]Key Laboratory of High-pricision Computation and Application of Quantum Field Theory of Hebei Province,Hebei University,Baoding 071002,China

出　　处：《Chinese Physics C》2020年第11期208-212,共5页中国物理C（英文版）

基　　金：Supported in part by Hebei Provincial Natural Science Foundation of China(A2014201068)。

摘　　要：We investigate whether the new horizon first law still holds in f(R,R^μνRμν)theory.For this complicated theory,we first determine the entropy of a black hole by using the Wald method,and then derive the energy of the black hole by using the new horizon first law,the degenerate Legendre transformation,and the gravitational field equations.For application,we consider the quadratic-curvature gravity,and first calculate the entropy and energy of a static spherically symmetric black hole,which are in agreement with the results obtained in the literature for a Schwarzschild-(A)dS black hole.

关 键 词：black hole energy ENTROPY new horizon first law 

分 类 号：P142[天文地球—天体物理] O414.1[天文地球—天文学]