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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Main Authors: Mikhailov, A. A., Efremov, N. N., Makarov, I. T., Nikolayeva, G. V., Struchkov, G. G.
Format: Text
Language:unknown
Published: arXiv 2004
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Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0405613
https://arxiv.org/abs/astro-ph/0405613
id ftdatacite:10.48550/arxiv.astro-ph/0405613
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spelling 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
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic 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
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