发现带电黑洞的霍金温度不仅依赖于时间 ，而且依赖于极角 。
We find Hawking temperature of a charged bl ack hole depends not only on the time;
但是，带电、旋转的黑洞——被称为“克尔-纽曼黑洞”——却展现出一个意想不到的扭曲。
But charged, rotating black holes - known as "kerr-newman black holes" - exhibit an unexpected twist.
自上世纪六十年代起，研究者们就开始研究在这种带电旋转的黑洞内的光子稳定轨道。
Since the 1960s, researchers have determined stable orbits for photons inside these charged, rotating black holes.
给出了带电蒸发黑洞发生自发辐射的能量条件。
The energy condition for the occurrence of the spontaneous radiation is obtained.
研究一般球对称带电蒸发黑洞视界附近粒子的能级交错，给出交错能级最大值的表达式，得出一般球对称带电蒸发黑洞非热辐射频率范围是随时间变化的结论。
We drew the conclusion that the frequency distribution of the non-thermal radiation from a general spherically-symmetric and charged evaporating black hole depended on the time.
研究一般球对称带电蒸发黑洞视界附近粒子的能级交错，给出交错能级最大值的表达式，得出一般球对称带电蒸发黑洞非热辐射频率范围是随时间变化的结论。
We drew the conclusion that the frequency distribution of the non-thermal radiation from a general spherically-symmetric and charged evaporating black hole depended on the time.
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