摘要
利用推广的Tortoise坐标,得到了在加速荷电黑洞视界邻域内Klein-Gorden方程的渐近解.求出了事件视界的位置和Hawking温度.结果表明:由于黑洞的加速作用,事件的形状不再是球对称的.在一定的条件下,所得结果退为Reissner-Nordstrm黑洞,Schwarzschile黑洞和F-Z加速黑洞结果.
Asymptotically solutions of the Klein-Gorden equation in region near event horizon of a uniformaly accelerating charged black hole are obtained by using generalized tortoise coordinate. The location of the event horizon and the Hawking temperature of the hole are given. In the appropriate limits, the results reduce to that of the Reissuer-Nordstrom, Schwarzschild and F-Z accelerating black hole.
出处
《湖南师范大学自然科学学报》
CAS
1996年第1期31-35,共5页
Journal of Natural Science of Hunan Normal University
基金
国家自然科学基金
关键词
HAWKING辐射
黑洞
K-G方程
加速作用
Hawking radiation
black hole
Klein-Gorden equation PACS 97. 60. Lf, 40. 60. tr