Primary cosmic ray energy spectrum in terms of the GAMMA muon data

被引：0

作者：

Garyaka, A. P. ^{[1
]}

Martirosov, R. M. ^{[1
]}

Ter-Antonyan, S. V. ^{[2
]}

Erlykin, A. D. ^{[3
]}

Nikolskaya, N. M. ^{[3
]}

Gallant, Y. A. ^{[4
]}

Jones, L. W. ^{[5
]}

Procureur, J. ^{[6
]}

机构：

[1] Yerevan Phys Inst, Yerevan 375036, Armenia

[2] Southern Univ, Dept Phys, Baton Rouge, LA USA

[3] Moscow Lebedev Phys Inst, Moscow, Russia

[4] Univ Montpellier 2, Lab Phys Theor & Astroparticules, F-34095 Montpellier 5, France

[5] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[6] Ctr Etud Nucl Bordeaux Gradignan, Gradignan, France

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2009年 / 196卷

关键词：

D O I：

10.1016/j.nuclphysbps.2009.09.073

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：

The energy spectrum of the primary cosmic rays is obtained by conversion from the truncated moon size spectrum of EAS studied with the GAMMA array. The previously observed dependence of E(0) on N(mu)(tr) at various zenith angles is used. It is shown that the present spectrum has the same structure ("bump") as the spectrum determined by another independent multi-parametric energy estimation method confirming that the "bump" structure is not produced by uncertainties in our methods.

引用

页码：387 / 390

页数：4

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