Modeling Source Spectra and Composition of Ultrahigh Energy Cosmic Rays
- 作者: Zirakashvili V.N.1, Klepach E.G.1, Rogovaya S.I.1, Ptuskin V.S.1
-
隶属关系:
- Pushkov Institute of Terrestrial Magnetism
- 期: 卷 82, 编号 6 (2019)
- 页面: 812-815
- 栏目: Elementary Particles and Fields
- URL: https://journals.rcsi.science/1063-7788/article/view/195018
- DOI: https://doi.org/10.1134/S1063778819660529
- ID: 195018
如何引用文章
详细
The inverse problem of cosmic ray transport of ultra-high energy cosmic rays is considered. The source spectrum and composition are derived based on the recent Auger data on energy spectrum, energy dependence of mean logarithm of atomic mass number and its variance. The dependence of results on the extrapolation of observable spectrum beyond energies 1020 eV is investigated.
作者简介
V. Zirakashvili
Pushkov Institute of Terrestrial Magnetism
编辑信件的主要联系方式.
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
E. Klepach
Pushkov Institute of Terrestrial Magnetism
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
S. Rogovaya
Pushkov Institute of Terrestrial Magnetism
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
V. Ptuskin
Pushkov Institute of Terrestrial Magnetism
Email: zirak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 108840
补充文件
