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Monte Carlo calculation of the atmospheric antinucleon flux

By T. Djemil, R. Attallah and J.-N. Capdevielle


International audienceThe atmospheric antiproton and antineutron energy spectra are calculated at float altitude using the CORSIKA package in a three-dimensional Monte Carlo simulation. The hadronic interaction is treated by the FLUKA code below 80 GeV/nucleon and NEXUS elsewhere. The solar modulation which is described by the force field theory and the geomagnetic effects are taken into account. The numerical results are compared with the BESS-2001 experimental data

Topics: [ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
Publisher: HAL CCSD
Year: 2008
DOI identifier: 10.1016/J.NUCLPHYSBPS.2009.09.070
OAI identifier: oai:HAL:in2p3-00730720v1
Provided by: Hal-Diderot
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