Clusters of Cosmic Rays above 4.10^19 eV

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dc.creatorMikhailov, A. A.
dc.creatorEfremov, N. N.
dc.date2005-07-28
dc.date.accessioned2026-07-07T02:18:21Z
dc.date.available2026-07-07T02:18:21Z
dc.descriptionArrival 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.
dc.description4 pages, 5 figures, the paper will be publish in Proc. ICRC, Pune, India, 2005
dc.identifierhttps://arxiv.org/abs/astro-ph/0507682
dc.identifierhttp://arxiv.org/abs/astro-ph/0507682
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9456
dc.subjectAstrophysics
dc.titleClusters of Cosmic Rays above 4.10^19 eV
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