黑洞熵的演化规律与热力学第三定律

The Evolution Law of Black Hole and the Third Law of Thermodynamics

将正、负能谱中黑洞能力学理分别应用于分析Schwarzchild(SW)黑洞.Kerr-Neuman(K-N)黑洞以及Sen黑洞的熵及其演化过程,对它们的对照分析结果表明:负能谱热力学对表征黑洞的熵及其演化规律和极限特征比Bekenstein热力学优越得多.

If the Bekenstein＇s thermodynamics is compared with the negative energy spectrum thermodynamics, what is actually the thermodynamic representation suitable for the real evolution process of black hole （or high density matter）？ To counter this problem in research, the excellent way is that to use these two thermodynamics to analyze the evolution process of typical stationary black hole, for example to use these two thermodynamics to analyze the Schwarzchild （SW） black hole, the Kerr-Neuman （K-N）black hole and the Sen black hole respectively, and then compare the results led by the Bekenstein＇s thermodynamics with the results led by the negative energy spectrum thermodynamics. Through the contrast analysis between these two thermodynamics it has been fully proven that the negative energy spectrum thermodynamics is an excellent thermodyn-amicrepresentation suitable for the real evolution process of black hole.