... 事件穹界 event horizon 狭义相对论 special relativity 广义相对论 general relativity ...
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事件穹界的史瓦西半径 Schwartzschild radius
在经典理论中,在黑洞的边界,即通常所称的事件穹界,光是不能逃逸的。
According to classical theory, at the boundary of a black hole-the so-called event horizon-light can no longer escape.
他们的计算显示崩塌恒星的事件穹界从来不会完全形成,或者至少对从远处观察黑洞的那位物理学家来说是不会完全形成的。
Their calculations suggest that the event horizon for collapsing stars never quite comes into existence, at least, not for the colleague watching from far away.
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