Input of nearby sources in spectra and anisotropy of ultrahigh energy cosmic rays

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Resumo

Propagation of ultrahigh energy cosmic rays from nearby sources was investigated. It is shown that observable spectrum, chemical composition and anisotropy at energies above 5 · 1018 eV can be explained in the model of one nearby source galaxy M87 with heavy chemical composition.

Sobre autores

V. Zirakashvili

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
of the Russian Academy of Sciences

Autor responsável pela correspondência
Email: zirak@izmiran.ru
Russia, 108840, Moscow

V. Ptuskin

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
of the Russian Academy of Sciences

Email: zirak@izmiran.ru
Russia, 108840, Moscow

S. Rogovaya

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation
of the Russian Academy of Sciences

Email: zirak@izmiran.ru
Russia, 108840, Moscow

Bibliografia

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Declaração de direitos autorais © В.Н. Зиракашвили, В.С. Птускин, С.И. Роговая, 2023