摘要
从Dirac四分量旋量方程出发,经广义Tortolse坐标变换,导出了变质量黑洞的视界面方程.在推导温度函数的过程中取消了传统的假设,并紧终获得了Dirac粒子的Hawkiny热谱公式.
The Location of event horizon of an evaporating charged black hole is obtained directly,starting from Dirac four quantum eguation,after generalized Tortoise coordinate Variatlon. In the courseof calculating the temperature on the event horizon, we are out of using the traditional supposal,and we ob-tain the Hawking radition formula of Dirac Partides.
出处
《山东师范大学学报(自然科学版)》
CAS
1994年第3期50-53,共4页
Journal of Shandong Normal University(Natural Science)
关键词
视界
温度函数
狄喇克粒子
黑洞
量子热效应
event horizon
temperature
generalized Tortoise coordina tetranslation
Dirac fourquantum equation