Journal
PHYSICAL REVIEW D
Volume 100, Issue 10, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.100.103018
Keywords
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Funding
- European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme [646623]
- U.S. Department of Energy [DE-SC0013880]
- U.S. National Science Foundation [PHY 1505990]
- KIT graduate school KSETA
- German Ministry of Education and Research (BMBF) [05A14VK1]
- Helmholtz Alliance for Astroparticle Physics (HAP) - Initiative and Networking Fund of the Helmholtz Association
- OE-Portugal, FCT, I. P. [CERN/FIS-PAR/0023/2017, IF/00820/2014/CP1248/CT0001]
- Mainz Institute for Theoretical Physics (MITP) of the DFG Cluster of Excellence PRISMA+ [39083149]
- U.S. Department of Energy (DOE) [DE-SC0013880] Funding Source: U.S. Department of Energy (DOE)
- Fundação para a Ciência e a Tecnologia [CERN/FIS-PAR/0023/2017, IF/00820/2014/CP1248/CT0001] Funding Source: FCT
Ask authors/readers for more resources
Muons and neutrinos from cosmic ray interactions in the atmosphere originate from decays of mesons in air-showers. SIBYLL-2.3c aims to give a precise description of hadronic interactions in the relevant phase space for conventional and prompt leptons in light of new accelerator data, including that from the LHC. SIBYLL is designed primarily as an event generator for use in simulation of extensive air showers. Because it has been tuned for forward physics as well as the central region, it can also be used to calculate inclusive fluxes. The purpose of this paper is to describe the use of SIBYLL-2.3c for calculation of fluxes of atmospheric leptons.
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