Clusters in Very High Energy Cosmic Rays

Simple item page
dc.creatorMikhailov, A. A.
dc.date2004-03-10
dc.date2004-03-19
dc.date.accessioned2026-07-07T02:12:34Z
dc.date.available2026-07-07T02:12:34Z
dc.descriptionArrival directions of cosmic rays with the energy E>4.10^{19} eV are analyzed by using data of the Yakutsk and AGASA (Japan) extensive air showers (EAS) arrays. It is supposed that the clusters can be formed as a result of decay of superheavy particles. The consequences of this supposition compare with experimental data.
dc.description3 pages, 2 figures, the paper will publish: Nauka i Technika, Yakutsk, 2004,N2; v4: minor conceptual changes
dc.identifierhttps://arxiv.org/abs/astro-ph/0403231
dc.identifierhttp://arxiv.org/abs/astro-ph/0403231
dc.identifierProc. 28-th RCRC, Moscow, 2004, 1306.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7498
dc.subjectAstrophysics
dc.titleClusters in Very High Energy Cosmic Rays
dc.typetext

Files

Collections

arXiv