匀加速带电黑洞热效应的研究  

The Study on Thermal Effect of a Uniformly Accelerating, Non-stationary,Charged Black Hole

作　　者：闫荣义[1] 杨兴强[1] 宋太平[1] 

机构地区：[1]南阳师范学院物理系,河南南阳473061

出　　处：《南都学坛（南阳师范学院学报）》2001年第3期36-38,共3页Academic Forum of Nandu

基　　金：河南省教委自然科学基金资助项目 (9816 0 0 0 1)

摘　　要：给出了匀加速荷电黑洞的Hawking效应和事件视界及相应温度。发现荷电黑洞的Hawking温度的变化不仅依赖于时间 ,而且依赖于极角 ,利用York方法讨论事件视界和Klein Gordon方程 ,结果得到进一步约化 ,物理意义也更加明显。The Hawking effect,event horizon and corresponding temperature of a uniformly accelerating,non stationary,charged black hole are given.It is found that the Hawking temperature of the charged black hole depends not only on the time,but also on the polar angle.The York′s method is used to discuss the event horizon and the K G equation,the result is more simplified and the physics meaning is more obvious.

关 键 词：黑洞 视界 温度 HAWKING效应 量子热效应 

分 类 号：P145.8[天文地球—天体物理] O413[天文地球—天文学]