| 黑洞熵应该满足能斯特定理 |
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| 引用本文： | 赵峥,朱建阳.黑洞熵应该满足能斯特定理[J].北京师范大学学报(自然科学版),1998,34(4):504-505. |
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| 作者姓名： | 赵峥 朱建阳 |
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| 作者单位： | 北京师范大学物理学系 |
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| 摘 要： |
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| 关 键 词： | 黑洞熵 能斯特定理 黑洞热力学 第三定律 |
BLACK HOLE ENTROPY SHOULD SATISFY NERNST THEOREM |
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| Zhao Zheng, Zhu Jianyang.BLACK HOLE ENTROPY SHOULD SATISFY NERNST THEOREM[J].Journal of Beijing Normal University(Natural Science),1998,34(4):504-505. |
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| Authors: | Zhao Zheng Zhu Jianyang |
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| Abstract: | The Kerr black hole is regarded as a thermodynamical system composed by two subsystems, the outer horizon (event horizon) and the inner horizon (Cauchy horizon). The black hole entropy is contributed by both the area of oilier horizon and the minus area of inner horizon. The entropy satisfies Nernst theorem. |
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| Keywords: | black hole entropy Nernst theorem black hole therrmodynamics the third law |
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