摘要
采用乌龟坐标变换,在视界面附近化简Klein-Gordon场方程,得到在视界面附近的辐射温度.用薄膜brick-wall模型,选择适当的截断因子和薄膜厚度,得到在视界面附近薄膜上的熵,结果表明黑洞熵与视界面积成正比.
By adopting tortoise coordinate transformation and changing the Klein-Gordon field equation to be wave equation near the vision interface, the radiation temperature of the black hole can be gotten. Counting the black hole's entropy with film brick-wall model indicates the entropy is in direct proportion to the vision interface area and the expression form is as simple as the static or steady state is.
出处
《重庆三峡学院学报》
2008年第3期88-91,共4页
Journal of Chongqing Three Gorges University
基金
重庆市教育委员会科学技术项目计划(KJ071111)