Clusters in Very High Energy Cosmic Rays
Arrival directions of cosmic rays with the energy E>4.10^{19} eV are analyzed by using data of the Yakutsk and AGASA (Japan) extensive air showers (EAS) arrays. It is supposed that the clusters can be formed as a result of decay of superheavy particles. The consequences of this supposition compar...
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ftdatacite:10.48550/arxiv.astro-ph/0403231 2023-05-15T18:45:20+02:00 Clusters in Very High Energy Cosmic Rays Mikhailov, A. A. 2004 https://dx.doi.org/10.48550/arxiv.astro-ph/0403231 https://arxiv.org/abs/astro-ph/0403231 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 article-journal Article ScholarlyArticle Text 2004 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0403231 2022-04-01T16:29:12Z Arrival directions of cosmic rays with the energy E>4.10^{19} eV are analyzed by using data of the Yakutsk and AGASA (Japan) extensive air showers (EAS) arrays. It is supposed that the clusters can be formed as a result of decay of superheavy particles. The consequences of this supposition compare with experimental data. : 3 pages, 2 figures, the paper will publish: Nauka i Technika, Yakutsk, 2004,N2; v4: minor conceptual changes Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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DataCite Metadata Store (German National Library of Science and Technology) |
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unknown |
topic |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Mikhailov, A. A. Clusters in Very High Energy Cosmic Rays |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
Arrival directions of cosmic rays with the energy E>4.10^{19} eV are analyzed by using data of the Yakutsk and AGASA (Japan) extensive air showers (EAS) arrays. It is supposed that the clusters can be formed as a result of decay of superheavy particles. The consequences of this supposition compare with experimental data. : 3 pages, 2 figures, the paper will publish: Nauka i Technika, Yakutsk, 2004,N2; v4: minor conceptual changes |
format |
Text |
author |
Mikhailov, A. A. |
author_facet |
Mikhailov, A. A. |
author_sort |
Mikhailov, A. A. |
title |
Clusters in Very High Energy Cosmic Rays |
title_short |
Clusters in Very High Energy Cosmic Rays |
title_full |
Clusters in Very High Energy Cosmic Rays |
title_fullStr |
Clusters in Very High Energy Cosmic Rays |
title_full_unstemmed |
Clusters in Very High Energy Cosmic Rays |
title_sort |
clusters in very high energy cosmic rays |
publisher |
arXiv |
publishDate |
2004 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0403231 https://arxiv.org/abs/astro-ph/0403231 |
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/0403231 |
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1766236374461054976 |