Flux of upward high-energy muons at the multi-component primary energy spectrum
| dc.creator | Ter-Antonyan, S. V. | |
| dc.creator | Biermann, P. L. | |
| dc.date | 2001-06-07 | |
| dc.date.accessioned | 2026-07-07T03:44:44Z | |
| dc.date.available | 2026-07-07T03:44:44Z | |
| dc.description | The atmospheric neutrino-induced upward muon flux are calculated by using the multi-component primary energy spectrum, CORSIKA EAS simulation code for the reproduction of the atmospheric neutrino spectra and improved parton model for charged-current cross sections. The results are obtained at 0.1-1000 TeV muon energy range and 0-89 degrees zenith angular range. | |
| dc.description | 4 pages, 5 figures, to appear in proceedings of 27th ICRC (Hamburg, August 7-15, 2001) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0106076 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0106076 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40682 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Flux of upward high-energy muons at the multi-component primary energy spectrum | |
| dc.type | text |