...场论；黑洞物理；非微扰QCD；手征对称性破缺。 [gap=1873]Keywords：Non-commutative quantum field theory; Black hole physics; Non-perturbative QCD; Chiral symmetry spontaneously breaking.
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timeline of black hole physics 黑洞物理学年表
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。
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