High Energy Particle Collisions in the vicinity of Naked Singularity
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arXiv
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| Main Authors: | , , , , |
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| Format: | Preprint |
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2023
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| _version_ | 1866915133452713984 |
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| author | Acharya, Kauntey Bambhaniya, Parth Joshi, Pankaj S. Pandey, Kshitij Patel, Vishva |
| author_facet | Acharya, Kauntey Bambhaniya, Parth Joshi, Pankaj S. Pandey, Kshitij Patel, Vishva |
| contents | In this paper, we investigate particle acceleration and high-energy collisions in the Joshi-Malafarina-Narayan (JMN-1) naked singularity, which, in the absence of an event horizon, allows infalling particles to turn back under specific angular momentum conditions. These outgoing particles can then collide with infalling ones, enabling the JMN-1 singularity to act as a natural high-energy particle accelerator. We derive the necessary expressions to compute the center-of-mass energy of two colliding particles and find that this energy can reach extremely high values, potentially even approaching Planck energy scales. We also explore the implications of these results, including the possible formation of microscopic black holes that could decay via Hawking radiation, releasing energy on the order of $10^{26} eV$ due to the extreme gravitational fields near the naked singularity. This scenario offers significant advantages. If horizonless compact objects exist in nature, these high-energy collisions could substantially influence the surrounding physical processes and might give rise to distinct observational signatures. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2303_16590 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | High Energy Particle Collisions in the vicinity of Naked Singularity Acharya, Kauntey Bambhaniya, Parth Joshi, Pankaj S. Pandey, Kshitij Patel, Vishva General Relativity and Quantum Cosmology In this paper, we investigate particle acceleration and high-energy collisions in the Joshi-Malafarina-Narayan (JMN-1) naked singularity, which, in the absence of an event horizon, allows infalling particles to turn back under specific angular momentum conditions. These outgoing particles can then collide with infalling ones, enabling the JMN-1 singularity to act as a natural high-energy particle accelerator. We derive the necessary expressions to compute the center-of-mass energy of two colliding particles and find that this energy can reach extremely high values, potentially even approaching Planck energy scales. We also explore the implications of these results, including the possible formation of microscopic black holes that could decay via Hawking radiation, releasing energy on the order of $10^{26} eV$ due to the extreme gravitational fields near the naked singularity. This scenario offers significant advantages. If horizonless compact objects exist in nature, these high-energy collisions could substantially influence the surrounding physical processes and might give rise to distinct observational signatures. |
| title | High Energy Particle Collisions in the vicinity of Naked Singularity |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2303.16590 |