A POSSIBLE GAMMA RAY PRIMARY AS THE HIGHEST ENERGY COSMIC RAYS

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KERMANI H.A.; FATEMI S.J.

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ISSN: 2588-4824

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Journal: Iranian Journal of Physics Research Year:2011 | Volume:10 | Issue:4 Page(s): 0-0

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Title

A POSSIBLE GAMMA RAY PRIMARY AS THE HIGHEST ENERGY COSMIC RAYS

Author(s)

KERMANI H.A. | FATEMI S.J. | Issue Writer Certificate

Keywords

MASS COMPOSITION

UHECR

MOUN-ELECTRON RATIO

Abstract

Muon-electron ratio and median zenith angle of Extensive Air Shower (EAS) is calculated for the energy range of 1019 to bigger than 1020 eV. The results are compared with the simulation work of Capdevielle et al. The results show a good correspondence with proton primary composition up to energy level of 7×1019 eV. In higher energies above GZK cut off, a considerable increase is calculated in cosmic primary photons. In addition, event frequency distribution above energy 7×1019 eV shows increasing concentration towards super galactic plane.

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APA: Copy

KERMANI, H.A., & FATEMI, S.J.. (2011). A POSSIBLE GAMMA RAY PRIMARY AS THE HIGHEST ENERGY COSMIC RAYS. IRANIAN JOURNAL OF PHYSICS RESEARCH, 10(4), 0-0. SID. https://sid.ir/paper/576340/en

Vancouver: Copy

KERMANI H.A., FATEMI S.J.. A POSSIBLE GAMMA RAY PRIMARY AS THE HIGHEST ENERGY COSMIC RAYS. IRANIAN JOURNAL OF PHYSICS RESEARCH[Internet]. 2011;10(4):0-0. Available from: https://sid.ir/paper/576340/en

IEEE: Copy

H.A. KERMANI, and S.J. FATEMI, “A POSSIBLE GAMMA RAY PRIMARY AS THE HIGHEST ENERGY COSMIC RAYS,” IRANIAN JOURNAL OF PHYSICS RESEARCH, vol. 10, no. 4, pp. 0–0, 2011, [Online]. Available: https://sid.ir/paper/576340/en

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