Very high energy cosmic ray particles from the Kerr black hole at the galaxy center
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arXiv
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| Hauptverfasser: | , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866917883336982528 |
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| author | Panella, Orlando Pacetti, Simone Immirzi, Giorgio Srivastava, Yogendra N. |
| author_facet | Panella, Orlando Pacetti, Simone Immirzi, Giorgio Srivastava, Yogendra N. |
| contents | Conventional general relativity supplies the notion of a vacuum tension and thus a maximum force $F_{max}=c^4/4G\approx\ 3\times 10^{43}$ Newtons, that is realized for a black hole. In conjunction with the Wilson area rule, we are thus led to the surface confinement of the mass of a black hole analogous to the surface confinement of quarks. The central result of our paper is that PeV scale protons exist on the surface of a Kerr black hole residing at our galactic center that is in concert with the HAWC Collaboration result of a PeVatron at the galactic center. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_01899 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Very high energy cosmic ray particles from the Kerr black hole at the galaxy center Panella, Orlando Pacetti, Simone Immirzi, Giorgio Srivastava, Yogendra N. High Energy Astrophysical Phenomena High Energy Physics - Phenomenology Conventional general relativity supplies the notion of a vacuum tension and thus a maximum force $F_{max}=c^4/4G\approx\ 3\times 10^{43}$ Newtons, that is realized for a black hole. In conjunction with the Wilson area rule, we are thus led to the surface confinement of the mass of a black hole analogous to the surface confinement of quarks. The central result of our paper is that PeV scale protons exist on the surface of a Kerr black hole residing at our galactic center that is in concert with the HAWC Collaboration result of a PeVatron at the galactic center. |
| title | Very high energy cosmic ray particles from the Kerr black hole at the galaxy center |
| topic | High Energy Astrophysical Phenomena High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2501.01899 |