摘要
在ｔ缓变情况下，直接用时间变量ｔ表述球对称荷电蒸发黑洞的动态特征，根据ＲｅｉｓｎｅｒＮｏｒｄｓｔｒ¨ｏｍ度规，采用ｔｏｒｔｏｉｓｅ坐标变换，用共形平直方法，研究了球对称荷电蒸发黑洞的热效应．
If the parameters which represent the spherically charged evaporating black hole are slowly varying the functions of time t, the non stationary characteristic is represented directly by t.According to the Reissner Nordstrm metric,the thermal effect of the spherically charged evaporating black hole is studied with the conformal flat method and the tortoise coordinate transformation.
出处
《四川师范学院学报（自然科学版）》
1997年第3期195-197,共3页
Journal of Sichuan Teachers College(Natural Science)
