然而，如果两者出现在视界的边缘，粒子或者黑洞都可能穿过视界再也不会来。
If, however, the pair appears on the edge of an event horizon, either particle or hole may wander across the horizon, never to return.
在柯西视界上，因为产生离心作用，粒子速度减慢，回到光速。
At this Cauchy horizon, because of the centrifugal forces involved, particles slow down back to the speed of light.
来自外面这个区域的粒子能落进去，越过活动视界，而将永远不能够离开。
Particles from outside this region can fall in, cross the event horizon, and will never be able to leave.
得到了粒子的能量不仪与粒子的质量有关，还与黑洞的时空结构及视界的变化有关。
We find that the energy of scalar particles is not only depends on its mass and angular momentum, but also is related to the structure of space-time and the variations of event horizon of black hole.
粒子的能量不仅与粒子的质量有关，还与黑洞的时空结构及视界的变化有关。
It is found that the energy of scalar particles is not only depends on their mass, but also on the structure of space-time and the variations of event horizon of Vaidya black hole.
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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