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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ftcern:oai:cds.cern.ch:738763 2023-05-15T18:45:25+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 http://cds.cern.ch/record/738763 eng eng http://cds.cern.ch/record/738763 astro-ph/0405613 oai:cds.cern.ch:738763 Astrophysics and Astronomy 2004 ftcern 2018-07-28T06:44:13Z 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. Other/Unknown Material Yakutsk CERN Document Server (CDS) Yakutsk |
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Open Polar |
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CERN Document Server (CDS) |
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ftcern |
language |
English |
topic |
Astrophysics and Astronomy |
spellingShingle |
Astrophysics and Astronomy 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 and Astronomy |
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. |
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 |
publishDate |
2004 |
url |
http://cds.cern.ch/record/738763 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
op_relation |
http://cds.cern.ch/record/738763 astro-ph/0405613 oai:cds.cern.ch:738763 |
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1766236461780172800 |