Why is black hole entropy affected by rotation?
Abstract It is well known that an asymptotically flat four-dimensional Kerr black hole has a smaller (specific) entropy than a Schwarzschild black hole of the same mass. We show here that the same is true if the temperature, rather than the mass, is held fixed; and we also show that an asymptoticall...
| 第一著者: | |
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| フォーマット: | 論文 |
| 言語: | English |
| 出版事項: |
SpringerOpen
2023-02-01
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| シリーズ: | Journal of High Energy Physics |
| 主題: | |
| オンライン･アクセス: | https://doi.org/10.1007/JHEP02(2023)072 |