Clusters of cosmic rays above 4.1019 eV

被引：0
|
作者：
Mikhailov, A. A. [1 ]
Efremov, N. N. [1 ]
Timofeev, V. [1 ]
机构：
[1] Yu G Shafer Inst Cosmophys Res & Aeron, Yakutsk 677980, Russia
来源：
Proceedings of the 29th International Cosmic Ray Conference Vol 7: HE 1.4 | 2005年
关键词：
D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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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页码：231 / 234
页数：4
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