Accreting black hole binaries are important objects to learn black hole physics.
吸积黑洞双星是认识黑洞物理的最重要目标之一。
However, if the supernova remnant exceeds three solar masses, conventional physics suggests a black hole should be left behind.
然而，如果超新星的残核大于三个太阳质量，按常规物理法则来说，就将成为黑洞。
We'd be able to connect a lot of the physics happening within the gaseous environment and accretion disk to the binary black hole merger to the gravitational radiation.
我们可以将很多发生在黑洞对合并时的气体环境和吸积盘里的物理过程与引力辐射联系起来。
The word singularity is borrowed from astrophysics: it refers to a point in space-time - for example, inside a black hole - at which the rules of ordinary physics do not apply.
奇点这个单词来自于天体物理学：它指的是时空中(例如黑洞内部)所有物理理论都失效的一点。
The singularity is located at the heart of a black hole, and is the place where the laws of physics and space-time break down.
奇点位于黑洞的中心，物理和时空法则在这里失去作用。
To understand what happens inside a black hole, we need to invent new physics.
要想理解黑洞内部发生的状况，我们需要发明新的物理方法。
Mercifully, the physics for the end state of a black hole is somewhat simpler.
幸运的是，对于黑洞演化最终状态的物理学描述可能相对更简单一些。
Mercifully, the physics for the end state of a black hole is somewhat simpler.
幸运的是，对于黑洞演化最终状态的物理学描述可能相对更简单一些。
应用推荐