Hawking Temperature and the Inverse-Radius Scale of the Horizon
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arXiv
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| Auteurs principaux: | , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866915106375335936 |
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| author | Good, Michael R. R. Ong, Yen Chin |
| author_facet | Good, Michael R. R. Ong, Yen Chin |
| contents | The Hawking temperature of a Schwarzschild black hole can be heuristically derived by identifying the temperature with the inverse radius of the horizon up to a multiplicative constant. This does not work for more general black holes such as the Kerr and Reissner-Nordström solutions. Expounding on the details of how it fails to work nevertheless uncovers interesting connections with the "spring constant" of black holes and with black hole thermodynamics. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_21114 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Hawking Temperature and the Inverse-Radius Scale of the Horizon Good, Michael R. R. Ong, Yen Chin General Relativity and Quantum Cosmology High Energy Physics - Theory The Hawking temperature of a Schwarzschild black hole can be heuristically derived by identifying the temperature with the inverse radius of the horizon up to a multiplicative constant. This does not work for more general black holes such as the Kerr and Reissner-Nordström solutions. Expounding on the details of how it fails to work nevertheless uncovers interesting connections with the "spring constant" of black holes and with black hole thermodynamics. |
| title | Hawking Temperature and the Inverse-Radius Scale of the Horizon |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2407.21114 |