Clusters of Cosmic Rays above 4.10^19 eV

A. A. Mikhailov; N. N. Efremov

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Clusters of Cosmic Rays above 4.10^19 eV

A. A. Mikhailov·N. N. Efremov

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Abstract

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.

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A. A. Mikhailov, N. N. Efremov. 2005-07-28. Clusters of Cosmic Rays above 4.10^19 eV. https://arxiv.org/abs/astro-ph/0507682

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