Clusters of Cosmic Rays above 4.10^19 eV

Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experi...

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Main Authors: Mikhailov, A A, Efremov, N N
Language:English
Published: 2005
Subjects:
Astrophysics and Astronomy
Yakutsk
Online Access:http://cds.cern.ch/record/860617
id ftcern:oai:cds.cern.ch:860617
record_format openpolar
spelling ftcern:oai:cds.cern.ch:860617 2023-05-15T18:45:24+02:00 Clusters of Cosmic Rays above 4.10^19 eV Mikhailov, A A Efremov, N N 2005-07-28 http://cds.cern.ch/record/860617 eng eng http://cds.cern.ch/record/860617 astro-ph/0507682 oai:cds.cern.ch:860617 Astrophysics and Astronomy 2005 ftcern 2018-07-28T07:36:23Z Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experimental data. Part of clusters with E>2.10^19 eV correlate with the nearest pulsars. The new effect is found - clusters intensify a feature of cosmic rays distribution. 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
Clusters of Cosmic Rays above 4.10^19 eV
topic_facet Astrophysics and Astronomy
description Arrival directions of cosmic rays with the energy E>4.10^19 eV are analyzed on the basis of the Yakutsk and AGASA extensive air shower arrays. It is supposed that the clusters can be formed as a result of fragmentation of superheavy nuclei. The consequences of this supposition compare with experimental data. Part of clusters with E>2.10^19 eV correlate with the nearest pulsars. The new effect is found - clusters intensify a feature of cosmic rays distribution.
author Mikhailov, A A
Efremov, N N
author_facet Mikhailov, A A
Efremov, N N
author_sort Mikhailov, A A
title Clusters of Cosmic Rays above 4.10^19 eV
title_short Clusters of Cosmic Rays above 4.10^19 eV
title_full Clusters of Cosmic Rays above 4.10^19 eV
title_fullStr Clusters of Cosmic Rays above 4.10^19 eV
title_full_unstemmed Clusters of Cosmic Rays above 4.10^19 eV
title_sort clusters of cosmic rays above 4.10^19 ev
publishDate 2005
url http://cds.cern.ch/record/860617
geographic Yakutsk
geographic_facet Yakutsk
genre Yakutsk
genre_facet Yakutsk
op_relation http://cds.cern.ch/record/860617
astro-ph/0507682
oai:cds.cern.ch:860617
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