如何“审查”一个黑洞奇点及其他
How to "Censor" a Black Hole Singularity and Beyond
摘要：
我们认为，黑洞可以被看作是一个引力光学元件，其内部的图像到地平线上。由于衍射限制，由引力波干涉形成的“艾里超球”不允许无限分辨率。因此，有效地审查了大地奇点。所提出的机制必须像克尔黑洞解那样包含内禀角动量。然而，假设一个静态的黑洞是从一个初始的克尔解发展而来的，那么根据熵增加原理，这个被破坏的超球就被委托给视界。这个丢失的关于系统分辨率的信息现在被包装在地平线上，这实际上提供了审查。如果该机制适用于早期宇宙，我们认为在CMB天空中看到的低方差圆是这种干涉图案的痕迹。
英文摘要：
We argue that a black hole can be viewed as a gravitational optical element that images its interior onto the horizon. Being diffraction limited the "Airy hyper-ball" that forms as a result of interference of gravitational waves, does not allow for infinite resolution. Thereby, effectively censoring the geodetic singularity. The mechanism proposed must imply intrinsic angular momentum as in the Kerr black hole solution. However, assuming that a static black hole develops from an initial Kerr solution the destroyed hyperball is delegated to the horizon by the principle of increasing entropy. This lost information about the system resolution is now packed on the horizon, which in effect provides the censorship. Should the mechanism be applicable to the early universe, we suggest that the low variance circles seen in the CMB sky are traces of such an interference pattern.
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