摘要
在Planck尺度下,采用WKB近似方法计算了Anti-de Sitter时空视界附近自旋为1/2,1,2等自旋场的熵密度、压强和能量密度.结果表明,Anti-de Sitter时空附近的热力学量不仅依赖于黑洞的特征和纯时空效应,还依赖于粒子的自旋效应和最小距离的尺度.
The state equations of spin fields near the Anti-de Sitter black holes are investigated by using WKB approximation under the Planck length. It is shown that the states equations not only depend on the characteristic of the black hole but also on the spin of the fields and the size of minimal length.
出处
《西南师范大学学报(自然科学版)》
CAS
CSCD
北大核心
2009年第6期40-44,共5页
Journal of Southwest China Normal University(Natural Science Edition)
基金
湛江师范学院科研基金资助项目(L0806)