AAfrag: Interpolation routines for Monte Carlo results on secondary production in proton-proton, proton-nucleus and nucleus-nucleus interactions
arXiv:1904.05129 · doi:10.1016/j.cpc.2019.08.001
Abstract
We provide a compilation of predictions of the QGSJET-II-04m model for the production of secondary species (photons, neutrinos, electrons, positrons, and antinucleons) that are covering a wide range of energies of the beam particles in proton-proton, proton-nucleus, nucleus-proton, and nucleus-nucleus reactions. The current version of QGSJET-II-04m has an improved treatment of the production of secondary particles at low energies: the parameters of the hadronization procedure have been fine-tuned, based on a number of recent benchmark experimental data, notably, from the LHCf, LHCb, and NA61 experiments. Our results for the production spectra are made publicly accessible through the interpolation routines AAfrag which are described below. Besides, we comment on the impact of Feynman scaling violation and isospin symmetry effects on antinucleon production.
9 pages, 7 eps figures; v2: minor cosmetic changes, accepted version
References in corpus (6)
- New calculation of antiproton production by cosmic ray protons and nuclei
- Measurement of antiproton production in collisions at GeV
- Neutrino yield from Galactic cosmic rays
- Nuclear enhancement of the photon yield in cosmic ray interactions
- Constraining high energy interaction mechanisms by studying forward hadron production at the LHC
- and production in collisions and the cosmic-ray flux ratio
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