Generalized Lemaître time for rotating and charged black holes and its near-horizon properties
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arXiv
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| author | Toporensky, A. V. Zaslavskii, O. B. |
| author_facet | Toporensky, A. V. Zaslavskii, O. B. |
| contents | We consider the behavior of the analogue of the Lemaitre time when a particle approaches the horizon of a rotating black hole. For the Kerr metric, the aforementioned time coincides with the Doran or Natario time but we consider a more general class of metrics. We scrutiny relationship between (i) its finiteness or divergence, (ii) the forward-in-time condition, (iii) the sign of a generalized momentum/energy, (iv) the validity of the principle of kinematic censorship. The latter notion means impossibility to release in any event an energy which is literally infinite. As a consequence, we obtain a new explanation, why collisions of two particles inside the horizon do not lead to infinite energy in their center of mass frame. The same results are also obtained for the Reissner-Nordström metric |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2509_12485 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Generalized Lemaître time for rotating and charged black holes and its near-horizon properties Toporensky, A. V. Zaslavskii, O. B. General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena High Energy Physics - Theory We consider the behavior of the analogue of the Lemaitre time when a particle approaches the horizon of a rotating black hole. For the Kerr metric, the aforementioned time coincides with the Doran or Natario time but we consider a more general class of metrics. We scrutiny relationship between (i) its finiteness or divergence, (ii) the forward-in-time condition, (iii) the sign of a generalized momentum/energy, (iv) the validity of the principle of kinematic censorship. The latter notion means impossibility to release in any event an energy which is literally infinite. As a consequence, we obtain a new explanation, why collisions of two particles inside the horizon do not lead to infinite energy in their center of mass frame. The same results are also obtained for the Reissner-Nordström metric |
| title | Generalized Lemaître time for rotating and charged black holes and its near-horizon properties |
| topic | General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena High Energy Physics - Theory |
| url | https://arxiv.org/abs/2509.12485 |