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| Main Authors: | , , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2404.16591 |
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| _version_ | 1866929327489155072 |
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| author | Wilhelmi, Emma de Oña López-Coto, Rubén Aharonian, Felix Amato, Elena Cao, Zhen Gabici, Stefano Hinton, Jim |
| author_facet | Wilhelmi, Emma de Oña López-Coto, Rubén Aharonian, Felix Amato, Elena Cao, Zhen Gabici, Stefano Hinton, Jim |
| contents | Ultrarelativistic particles called cosmic rays permeate the Milky Way, propagating through the Galactic turbulent magnetic fields. The mechanisms under which these particles increase their energy can be reasonably described by current theories of acceleration and propagation of cosmic rays. There are, however, still many open questions as to how to reach petaelectronvolt (PeV) energies, the maximum energy believed to be attained in our Galaxy, and in which astrophysical sources (dubbed {\it PeVatrons}) this ultra-high energy acceleration happens. In this article, we describe the theoretical conditions for plasma acceleration to these energies, and the Galactic sources in which these conditions are possible. These theoretical predictions are then confronted with the latest experimental results, summarising the state-of-the-art of our current knowledge of PeVatrons. We finally describe the prospects to keep advancing the understanding of these elusive objects, still unidentified more than one hundred years after the discovery of cosmic rays. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_16591 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The hunt of PeVatrons as the origin of the most energetic photons observed in our Galaxy Wilhelmi, Emma de Oña López-Coto, Rubén Aharonian, Felix Amato, Elena Cao, Zhen Gabici, Stefano Hinton, Jim High Energy Astrophysical Phenomena Ultrarelativistic particles called cosmic rays permeate the Milky Way, propagating through the Galactic turbulent magnetic fields. The mechanisms under which these particles increase their energy can be reasonably described by current theories of acceleration and propagation of cosmic rays. There are, however, still many open questions as to how to reach petaelectronvolt (PeV) energies, the maximum energy believed to be attained in our Galaxy, and in which astrophysical sources (dubbed {\it PeVatrons}) this ultra-high energy acceleration happens. In this article, we describe the theoretical conditions for plasma acceleration to these energies, and the Galactic sources in which these conditions are possible. These theoretical predictions are then confronted with the latest experimental results, summarising the state-of-the-art of our current knowledge of PeVatrons. We finally describe the prospects to keep advancing the understanding of these elusive objects, still unidentified more than one hundred years after the discovery of cosmic rays. |
| title | The hunt of PeVatrons as the origin of the most energetic photons observed in our Galaxy |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2404.16591 |