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
Language:English
Published: 2004
Subjects:
Online Access:http://cds.cern.ch/record/738763
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spelling 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
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id 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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