黑洞、熵和第三定律
Black Holes, Entropy and the Third Law
摘要：
经典热力学定律和黑洞热力学定律之间存在着完美的对应关系，除了黑洞热力学显然不符合第三定律。经典热力学第三定律意味着，当绝对温度T接近零时，熵S也接近零。这一讨论是基于作者在1995年发表的工作的一部分，该工作表明，通过将内事件视界的面积作为负熵（负熵）的度量，经典热力学第三定律的最一般形式得到满足。
英文摘要：
There would be a perfect correspondence between the laws of classical thermodynamics and black hole thermodynamics, except for the apparent failure of black hole thermodynamics to correspond to the Third Law. The classical Third Law of Thermodynamics entails that as the absolute temperature, T, approaches zero, the entropy, S, also approaches zero. This discussion is based upon part of the work published by the author in 1995 that demonstrated that the most general form of the classical Third Law of Thermodynamics is satisfied by treating the area of the inner-event horizon as a measure of negative-entropy (negentropy).
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
