Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum

被引：1

作者：

Aloisio, Roberto ^{[1
,2
]}

机构：

[1] Gran Sasso Sci Inst, Laquila, Italy

[2] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila, Italy

来源：

7TH ROMA INTERNATIONAL CONFERENCE ON ASTROPARTICLE PHYSICS (RICAP18) | 2019年 / 209卷

关键词：

D O I：

10.1051/epjconf/201920901018

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The physics of Ultra High Energy Cosmic Rays will be reviewed, discussing the latest experimental results and theoretical models aiming at explaining the observations in terms of spectra, mass composition and possible sources. It will be also discussed the emission of secondary particles such as neutrinos and gamma rays produced by the interaction of Ultra High Energy Cosmic Rays with astrophysical photon backgrounds. The content of the present proceeding paper is mainly based on the review papers [1, 2].

引用

页数：6

共 50 条

[1] The origin of high energy cosmic rays displayed by the energy spectrum and elemental composition
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ACTA PHYSICA POLONICA B, 2000, 31 (02): : 323 - 334
[2] On origin of ultra high energy cosmic rays
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[3] On origin of ultra high energy cosmic rays
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[4] The origin of ultra high energy cosmic rays
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[8] Ultra High Energy Cosmic Rays: Anisotropies and spectrum
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[9] Propagation and Energy Spectrum of Ultra High Energy Cosmic Rays
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[10] ENERGY SPECTRUM AND COMPOSITION OF COSMIC RAYS OF GALACTIC AND METAGALACTIC ORIGIN
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