Composition of Cosmic Rays with the Energy more than 4x10^{19} eV
Arrival directions of extensive air showers by using world data are considered. It is found that the shower distribution in zenith angle at the energies E>10^{19} eV and E>4x10^{19} eV differs from each other. By our estimations, the shower with E>10^{20} eV at the Sugar array was not regis...
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| Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0312468 https://arxiv.org/abs/astro-ph/0312468 |
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ftdatacite:10.48550/arxiv.astro-ph/0312468 2023-05-15T18:44:59+02:00 Composition of Cosmic Rays with the Energy more than 4x10^{19} eV Mikhailov, A. A. 2003 https://dx.doi.org/10.48550/arxiv.astro-ph/0312468 https://arxiv.org/abs/astro-ph/0312468 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2003 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0312468 2022-04-01T16:40:46Z Arrival directions of extensive air showers by using world data are considered. It is found that the shower distribution in zenith angle at the energies E>10^{19} eV and E>4x10^{19} eV differs from each other. By our estimations, the shower with E>10^{20} eV at the Sugar array was not registered. The mass composition of very high-energy cosmic rays has been estimated. It is shown that E>4x10^{19} eV cosmic rays are, most likely, super heavy nuclei with charge Z>26. : 5 pages, 4 figures. Contributed talk presented at 28-th ICRC, Thusuba, Aug., 2003; Sem. Inst. Nucl. Phys., Lodz, Oct. 2003; Sem.Piatkowe OAUJ,Krakov, Oct. 2003. Accepted in journal "Nauka and Tecnika in Yakutia", 2004, n.1, Yakutsk Report Yakutia Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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Open Polar |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
| language |
unknown |
| topic |
Astrophysics astro-ph FOS Physical sciences |
| spellingShingle |
Astrophysics astro-ph FOS Physical sciences Mikhailov, A. A. Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| topic_facet |
Astrophysics astro-ph FOS Physical sciences |
| description |
Arrival directions of extensive air showers by using world data are considered. It is found that the shower distribution in zenith angle at the energies E>10^{19} eV and E>4x10^{19} eV differs from each other. By our estimations, the shower with E>10^{20} eV at the Sugar array was not registered. The mass composition of very high-energy cosmic rays has been estimated. It is shown that E>4x10^{19} eV cosmic rays are, most likely, super heavy nuclei with charge Z>26. : 5 pages, 4 figures. Contributed talk presented at 28-th ICRC, Thusuba, Aug., 2003; Sem. Inst. Nucl. Phys., Lodz, Oct. 2003; Sem.Piatkowe OAUJ,Krakov, Oct. 2003. Accepted in journal "Nauka and Tecnika in Yakutia", 2004, n.1, Yakutsk |
| format |
Report |
| author |
Mikhailov, A. A. |
| author_facet |
Mikhailov, A. A. |
| author_sort |
Mikhailov, A. A. |
| title |
Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| title_short |
Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| title_full |
Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| title_fullStr |
Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| title_full_unstemmed |
Composition of Cosmic Rays with the Energy more than 4x10^{19} eV |
| title_sort |
composition of cosmic rays with the energy more than 4x10^{19} ev |
| publisher |
arXiv |
| publishDate |
2003 |
| url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0312468 https://arxiv.org/abs/astro-ph/0312468 |
| geographic |
Yakutsk |
| geographic_facet |
Yakutsk |
| genre |
Yakutia Yakutsk |
| genre_facet |
Yakutia Yakutsk |
| op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
| op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0312468 |
| _version_ |
1766235888628531200 |