变加速带电黑洞热效应的讨论  

THE DISCUSSION ON THERMAL EFFECT OF NONUNIFORMLY RECTILINEARLY ACCELERATING AND CHARGED BLACK HOLE

作　　者：杨成全[1,2] 杨成全[1,2] 赵峥 

机构地区：[1]北京师范大学物理学系,北京100875 [2]雁北师范学院物理学系,大同037000

出　　处：《北京师范大学学报（自然科学版）》1999年第4期455-458,共4页Journal of Beijing Normal University(Natural Science)

基　　金：国家自然科学基金!19773003

摘　　要：给出了变加速直线运动带电黑洞的ＨＭ效应和事件视界以及相应的温度．发现带电黑洞的Ｈａｗｋｉｎｇ温度不仅依赖于时间，而且依赖于极角．利用Ｙｏｒｋ的方法讨论事件视界和Ｋｌｅｉｎ－Ｇｏｒｄｏｎ方程，结果得到进一步约化，物理意义也更为明显．The Hawking effect, event horizon and corrponding temperature of a nonuniformly rectilineariy acctating and charged black hole are given. It is found that Hawkingtemperature of the charged black hole depends not ohly on the the, but also on the polar angle. The York's odhod is used to discuss the event horizon and the K-G equation, the resultis simplified and the physics meaning is more obvious.

关 键 词：黑洞 视界 温度 HAWKING效应 带电黑洞 热效应 

分 类 号：P145.8[天文地球—天体物理]