Fluxes of Atmospheric Leptons at 600 GeV - 60 TeV
| dc.creator | Chirkin, Dmitry | |
| dc.date | 2004-07-07 | |
| dc.date.accessioned | 2026-07-25T19:03:40Z | |
| dc.description | The atmospheric muon flux is generated with CORSIKA 6.030 (using QGSJET high-energy interaction model) and fitted with the formula from Gaisser (1990). Spectra and mass distribution of primaries were taken according to the poli-gonato model of Horandel (2003). A convenient parameterization of the cos(th)->cos(th*) correction, originally tabulated in Volkova (1969), is presented. This correction, together with muon energy losses and decay, is shown to significantly improve the fit to the simulated data. | |
| dc.description | routines with corrections are available at http://amanda.berkeley.edu/~dima/work/CORSIKA/ | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0407078 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0407078 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/61075 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Fluxes of Atmospheric Leptons at 600 GeV - 60 TeV | |
| dc.type | text |