Clusters of Cosmic Rays above 4.10^19 eV
Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experi...
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arXiv
2005
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| Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0507682 https://arxiv.org/abs/astro-ph/0507682 |
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ftdatacite:10.48550/arxiv.astro-ph/0507682 2023-05-15T18:45:25+02:00 Clusters of Cosmic Rays above 4.10^19 eV Mikhailov, A. A. Efremov, N. N. 2005 https://dx.doi.org/10.48550/arxiv.astro-ph/0507682 https://arxiv.org/abs/astro-ph/0507682 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2005 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0507682 2022-04-01T16:15:19Z Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experimental data. Part of clusters with E>2.10^19 eV correlate with the nearest pulsars. The new effect is found - clusters intensify a feature of cosmic rays distribution. : 4 pages, 5 figures, the paper will be publish in Proc. ICRC, Pune, India, 2005 Report Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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Open Polar |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
| language |
unknown |
| topic |
Astrophysics astro-ph FOS Physical sciences |
| spellingShingle |
Astrophysics astro-ph FOS Physical sciences Mikhailov, A. A. Efremov, N. N. Clusters of Cosmic Rays above 4.10^19 eV |
| topic_facet |
Astrophysics astro-ph FOS Physical sciences |
| description |
Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experimental data. Part of clusters with E>2.10^19 eV correlate with the nearest pulsars. The new effect is found - clusters intensify a feature of cosmic rays distribution. : 4 pages, 5 figures, the paper will be publish in Proc. ICRC, Pune, India, 2005 |
| format |
Report |
| author |
Mikhailov, A. A. Efremov, N. N. |
| author_facet |
Mikhailov, A. A. Efremov, N. N. |
| author_sort |
Mikhailov, A. A. |
| title |
Clusters of Cosmic Rays above 4.10^19 eV |
| title_short |
Clusters of Cosmic Rays above 4.10^19 eV |
| title_full |
Clusters of Cosmic Rays above 4.10^19 eV |
| title_fullStr |
Clusters of Cosmic Rays above 4.10^19 eV |
| title_full_unstemmed |
Clusters of Cosmic Rays above 4.10^19 eV |
| title_sort |
clusters of cosmic rays above 4.10^19 ev |
| publisher |
arXiv |
| publishDate |
2005 |
| url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0507682 https://arxiv.org/abs/astro-ph/0507682 |
| geographic |
Yakutsk |
| geographic_facet |
Yakutsk |
| genre |
Yakutsk |
| genre_facet |
Yakutsk |
| op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
| op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0507682 |
| _version_ |
1766236461041975296 |