On some peculiarities of cosmic gamma-radiation in the energy range ~ 10^14 - 10^15 eV
| dc.creator | Barnaveli, T. T. | |
| dc.creator | Barnaveli Jr, T. T. | |
| dc.creator | Eristavi, N. A. | |
| dc.creator | Khaldeeva, I. V. | |
| dc.date | 2006-07-15 | |
| dc.date.accessioned | 2026-07-07T07:15:42Z | |
| dc.date.available | 2026-07-07T07:15:42Z | |
| dc.description | The distribution of EAS hadronic component energy fluxes through the ionization calorimeter in the primary energy range ~ 3x10^13 - 10^16 eV is considered. The EAS, carrying the zero or the minimal flux of the hadron component energy are extracted. The conclusion supports the existence of izotropic gamma-radiation in the primary energy region E_0 ~ 1x10^14 - 2x10^15 eV. This radiation has a spectrum of a form, close to the bell-like one, with the maximum at E_0 ~ 2.2x10^14 ev and with an additional local maximum at E_0 ~ 1.6x10^15 eV. | |
| dc.description | 8 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0607352 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0607352 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/113308 | |
| dc.subject | Astrophysics | |
| dc.title | On some peculiarities of cosmic gamma-radiation in the energy range ~ 10^14 - 10^15 eV | |
| dc.type | text |