Bekenstein-Hawking Cosmological Entropy and Correction Term Corresponding Cosmological Horizon of Rotating and Charged Black String  

作　　者：ZHAO Ren WU Yue-Qin ZHANG Li-Chun LI Huai-Fan 

机构地区：[1]Institute of Theoretical Physics, Shanxi Datong University, Datong 037009, China [2]Department of Physics, Shanxi Datong University, Datong 037009, China

出　　处：《Communications in Theoretical Physics》2009年第8期264-268,共5页理论物理通讯（英文版）

基　　金：Supported by the Shanxi Natural Science Foundation of China under Grant No.2006011012;the Doctoral Scientific Research Starting Foundation of Shanxi Datong University

摘　　要：Utilizing the quantum statistical method and applying the new state density equation motivated by generalized uncertainty principle in quantum gravitaty, we avoid the difficulty in solving wave equation and directly calculate the partition function of bosonic and fermionic field on the background of rotating and charged black string. Then near the cosmological horizon, entropies of bosonic and fermionic field are calculated on the background of black string. When constant A introduced in generalized uncertainty principle takes a proper value, we derive Bekenstein- Hawking entropy and the correction value corresponding cosmologicaJ horizon on the background of rotating and charged black string. Because we use the new state density equation, in our calculation there are not divergent term and small mass approximation in the original brick-wall method. From the view of quantum statistic mechanics, the correction value to Bekenstein-Hawking entropy of the black string is derived. It makes people deeply understand the correction value to the entropy of the black string cosmological horizon in non-spherical coordinate spacetime.

关 键 词：quantum statistics nonspherical symmetry spacetime generalized uncertainty principle entropy corresponding black string cosmological horizon 

分 类 号：P159[天文地球—天文学] TP311.1[自动化与计算机技术—计算机软件与理论]