论文标题
黑洞热力学的第二定律
Second law of black hole thermodynamics
论文作者
论文摘要
如果在Bekenstein-Hawking区域中为Schwarzschild黑洞进行简单的into镜，将被“负”量子条件熵取代，它相对于外部的正面能量的量子纠缠量化了量子纠缠，相对于其外部的正能量粒子，这是一个悖论，是hawking radiation for for Black for for Black for iSics and vents Isics and Quant iSics and pot-nake andics and pot-nakic andics insics and vent isicics andics sick andics andics isicics andics isics。但是，没有办法通过实验来判断黑洞确实采用了哪个区域法。在这里，有了无头发的猜想，我们为修改区法律的任何黑洞而不是Bekenstein从最初的区域定律中获得的任何黑洞，而不是黑洞的热力学第二定律的完美图片。与Bekenstein的望远镜相比，第二定律是通过事件范围望远镜进行测试的。如果确认了这一点，则可以将修改的区域定律提升为物理学基础方程的第一个例子，而没有量子信息的概念就无法描述。
If simple entropy in the Bekenstein-Hawking area law for a Schwarzschild black hole is replaced with 'negative' quantum conditional entropy, which quantifies quantum entanglement, of positive-energy particles of the black hole relative to its outside, a paradox with the original pair-creation picture of Hawking radiation, the first law for black hole mechanics and quantum mechanics is resolved. However, there was no way to judge experimentally which area law is indeed adopted by black holes. Here, with the no-hair conjecture, we derive the perfect picture of a second law of black hole thermodynamics for any black hole from the modified area law, rather than Bekenstein's generalized one from the original area law. The second law is testable with an event horizon telescope, in contrast to Bekenstein's. If this is confirmed, the modified area law could be exalted to the first example of fundamental equations in physics which cannot be described without the concept of quantum information.
