Cosmic ray muons and muon bremsstrahlung gammas at very high energies in the atmosphere

被引：0
|
作者：
Volkova, L. V. [1 ]
机构：
[1] RAS, Inst Nucl Res, Moscow 117312, Russia
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2012年 / 221卷
基金：
俄罗斯基础研究基金会;
关键词：
D O I：
10.1016/j.nuclphysbps.2011.10.055
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
Fluxes of cosmic ray muons and production functions of muon bremsstrahlung gammas and of gammas from pi degrees-decays are calculated at different angles and levels in the atmosphere (3*10(6)-10(12) GeV). It is shown that charm and j/psi production in nucleon- nucleus interactions is to be taken into account when EAS data are interpreted. The calculations are based on data from experiments on accelerators and their extrapolation to higher energies.
引用
收藏
页码：411 / 411
页数：1
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