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：

暂无

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.

引用

页码：231 / 234

页数：4

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