The origin of the cosmic ray
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2026
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| _version_ | 1866901997545848832 |
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| author | Tian, Zhenyuan Tian, yunchuan |
| author_facet | Tian, Zhenyuan Tian, yunchuan |
| contents | <p>We found that solar neutrinos with energy of about 10 Mev have perihelion effect, and<br>protons with energy above Gev of AMS-02 also have perihelion effect, so it is believed that<br>solar energy produces cosmic rays with energy above Gev. We propose a neutrino collision<br>model for the origin of cosmic rays. This model can reasonably explain the problem that the<br>proton flow in cosmic rays is much greater than the electron flow.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_19313609 |
| institution | Zenodo |
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| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The origin of the cosmic ray Tian, Zhenyuan Tian, yunchuan Cosmic rays Origin of cosmic rays Neutrino collision model Solar cosmic rays High-energy particles <p>We found that solar neutrinos with energy of about 10 Mev have perihelion effect, and<br>protons with energy above Gev of AMS-02 also have perihelion effect, so it is believed that<br>solar energy produces cosmic rays with energy above Gev. We propose a neutrino collision<br>model for the origin of cosmic rays. This model can reasonably explain the problem that the<br>proton flow in cosmic rays is much greater than the electron flow.</p> |
| title | The origin of the cosmic ray |
| topic | Cosmic rays Origin of cosmic rays Neutrino collision model Solar cosmic rays High-energy particles |
| url | https://doi.org/10.5281/zenodo.19313609 |