High-energy photons from Gamma-Ray Bursts, but no neutrinos
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arXiv
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| Format: | Preprint |
| Published: |
2025
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| _version_ | 1866918160536436736 |
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| author | De Rújula, A. |
| author_facet | De Rújula, A. |
| contents | The Cannon-Ball model of Gamma-Ray Bursts and their afterglows--described in the text and in innumerable previous occasions--is extremely successful and predictive. In a few intrinsically bright GRBs, gamma-rays with energies in the TeV range have been observed. The CB model, I argue, has no difficulty in describing the origin and approximate properties of these high-energy gamma rays and the extreme difficulty of observing their accompanying neutrinos. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2510_12634 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | High-energy photons from Gamma-Ray Bursts, but no neutrinos De Rújula, A. High Energy Physics - Phenomenology High Energy Astrophysical Phenomena The Cannon-Ball model of Gamma-Ray Bursts and their afterglows--described in the text and in innumerable previous occasions--is extremely successful and predictive. In a few intrinsically bright GRBs, gamma-rays with energies in the TeV range have been observed. The CB model, I argue, has no difficulty in describing the origin and approximate properties of these high-energy gamma rays and the extreme difficulty of observing their accompanying neutrinos. |
| title | High-energy photons from Gamma-Ray Bursts, but no neutrinos |
| topic | High Energy Physics - Phenomenology High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2510.12634 |