Deficit of Ultrahigh Energy Extensive Air Showers
Arrival directions of extensive air showers by using world data are considered. It is shown that distributions of showers in zenith angle at E>10^{19}eV and E>4.10^{19}eV differ from each other. On this basis the conclusions are made: the estimation of the energy of inclined showers at E>4....
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Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0405613 https://arxiv.org/abs/astro-ph/0405613 |
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ftdatacite:10.48550/arxiv.astro-ph/0405613 2023-05-15T18:45:26+02:00 Deficit of Ultrahigh Energy Extensive Air Showers Mikhailov, A. A. Efremov, N. N. Makarov, I. T. Nikolayeva, G. V. Struchkov, G. G. 2004 https://dx.doi.org/10.48550/arxiv.astro-ph/0405613 https://arxiv.org/abs/astro-ph/0405613 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/0405613 2022-04-01T16:38:37Z Arrival directions of extensive air showers by using world data are considered. It is shown that distributions of showers in zenith angle at E>10^{19}eV and E>4.10^{19}eV differ from each other. On this basis the conclusions are made: the estimation of the energy of inclined showers at E>4.10^{19}eV at Yakutsk and AGASA arrays is incorrect; the cosmic ray spectrum is not break up and most likely continued up to E=10^{20}eV and higher. It is found that ultrahigh energy cosmic rays are, probably, superheavy nuclei. : 4 pages, 4 figures. The paper will be published in Proc. 28-th Russian conf. on cosm. rays, Moscow, 2004 Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Mikhailov, A. A. Efremov, N. N. Makarov, I. T. Nikolayeva, G. V. Struchkov, G. G. Deficit of Ultrahigh Energy Extensive Air Showers |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
Arrival directions of extensive air showers by using world data are considered. It is shown that distributions of showers in zenith angle at E>10^{19}eV and E>4.10^{19}eV differ from each other. On this basis the conclusions are made: the estimation of the energy of inclined showers at E>4.10^{19}eV at Yakutsk and AGASA arrays is incorrect; the cosmic ray spectrum is not break up and most likely continued up to E=10^{20}eV and higher. It is found that ultrahigh energy cosmic rays are, probably, superheavy nuclei. : 4 pages, 4 figures. The paper will be published in Proc. 28-th Russian conf. on cosm. rays, Moscow, 2004 |
format |
Text |
author |
Mikhailov, A. A. Efremov, N. N. Makarov, I. T. Nikolayeva, G. V. Struchkov, G. G. |
author_facet |
Mikhailov, A. A. Efremov, N. N. Makarov, I. T. Nikolayeva, G. V. Struchkov, G. G. |
author_sort |
Mikhailov, A. A. |
title |
Deficit of Ultrahigh Energy Extensive Air Showers |
title_short |
Deficit of Ultrahigh Energy Extensive Air Showers |
title_full |
Deficit of Ultrahigh Energy Extensive Air Showers |
title_fullStr |
Deficit of Ultrahigh Energy Extensive Air Showers |
title_full_unstemmed |
Deficit of Ultrahigh Energy Extensive Air Showers |
title_sort |
deficit of ultrahigh energy extensive air showers |
publisher |
arXiv |
publishDate |
2004 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0405613 https://arxiv.org/abs/astro-ph/0405613 |
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/0405613 |
_version_ |
1766236486560120832 |