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1·Therefore, you can never escape from inside the event horizon.

逃离视界中心，没有东西能逃离。

2·The trailing edge of the second pulse, therefore, also ACTS as an event horizon.

因此，第二个脉冲的后缘地带也发挥了视界的作用。

3·If m is the mass of the sun, the radius of the event horizon is three kilometers.

视界的半径就是，3公里，若m是太阳的三倍重。

4·If you tell me what m is, I will tell you what the radius of the event horizon is.

我会告诉你们，视界的，半径大小，这里我加快一点。

5·It's like looking at a mass accelerated past the event horizon of a black hole.

就象在看一个大规模加速通过一个黑洞的视界。

6·The general event horizon formula of black hole is given from null hypersurface equation.

从零曲面方程出发，导出了黑洞视界面的普遍公式。

7·They have not only an outer event horizon but also an inner horizon, called a Cauchy horizon.

它们不仅有一个外边界，还有一个内边界，称为“柯西”视界。

8·In effect, an event horizon has formed in the river, preventing waves from making their way out.

实际上，视界已经在河中形成了，并阻止水波流动。

9·However an observer at the event horizon would think that the man never reached the center at all.

然而事界的观察者认为那个人根本不能到达中心。

10·This spinning area surrounding the event horizon is called the ergosphere and has an ellipsoidal shape.

这活动视界周围旋转的区域是所谓的能层而具有椭圆形。

视界

1·The trailing edge of the second pulse, therefore, also ACTS as an event horizon.

因此，第二个脉冲的后缘地带也发挥了视界的作用。

2·To be sucked in by a black hole, you need to reach its event horizon, the one-way boundary beyond which nothing can escape.

要被一个黑洞吸入，你必须抵达它的视界，即：超过这个边界任何都无法逃离的单程边界。

3·But once inside the event horizon (the surface of a black hole) it is never possible to communicate with the outside.

但是，一旦进入视界(黑洞的表面)，就绝无可能与外界交流了。

4·This spinning area surrounding the event horizon is called the ergosphere and has an ellipsoidal shape.

这活动视界周围旋转的区域是所谓的能层而具有椭圆形。

5·According to theory, the event horizon of a black hole that is not spinning is spherical, and its singularity is (informally speaking) a single point.

依照理论，不旋转的黑洞活动视界是球形的，而且它的奇异点是(非正式说法)是单一点。