aafragpy

aafragpy

Python implementation of the AAFrag secondary particle production model (based on QGSJET-II-04m) with adaptive curve-morphing interpolation. The package provides fast, vectorized reconstruction of differential production cross-sections and spectra from high-energy hadronic interactions while preserving the original tabulated Monte Carlo precision.

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Features

• Secondary Products: Photons (γ), electrons and positrons (e±), neutrinos (ν_e, ν̄_e, ν_μ, ν̄_μ, ν_all), nucleons (p, p̄, n, n̄), and light antinuclei (d̄, ³Hē).
• Collision Systems: p–p, p–He, He–p, He–He, heavy projectile ions (C, Al, Fe) on proton targets, and antiproton-induced channels (p̄–p, p̄–He).
• Broad Energy Range: Tabulated interactions from kinematic thresholds (hundreds of MeV / low GeV) up to hundreds of PeV / EeV.
• Integrated Alternative Models: Built-in parameterizations for p–p interactions from Kamae et al. (2006) and Kafexhiu et al. (2014).

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Installation

Install aafragpy via pip:

pip install aafragpy

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Interactive Tutorial

A step-by-step walkthrough of the package API and spectral calculations is available in the Jupyter Notebook tutorial.

You can launch and run the interactive tutorial directly in Google Colab:

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Citation Policy

Important Notice on Citations:
If you use aafragpy in your scientific work, please cite both the aafragpy package paper and the corresponding original AAFrag / Monte Carlo data publications. Proper attribution to the original cross-section calculations ensures continued support and development of hadronic interaction models.

1. Python Package Citation

• S. Koldobskiy, M. Kachelrieß, A. Lskavyan, A. Neronov, S. Ostapchenko, and D. V. Semikoz,
  “Energy spectra of secondaries in proton-proton interactions,”
  Phys. Rev. D 104, 123027 (2021), arXiv:2110.00496.

2. Original AAFrag Model & Data Calculations

• AAfrag 2.0 (v2.02 Data Tables & Antinuclei):
  M. Kachelrieß, S. Ostapchenko, and J. Tjemsland,
  “AAfrag 2.01: Interpolation routines for Monte Carlo results on secondary production including light antinuclei in hadronic interactions,”
  Comput. Phys. Commun. 287, 108698 (2023), arXiv:2206.00998.

• AAfrag 1.0 (Original QGSJET-II-04m Tabulations):
  M. Kachelrieß, I. V. Moskalenko, and S. Ostapchenko,
  “AAfrag: Interpolation routines for Monte Carlo results on secondary production in proton-proton, proton-nucleus and nucleus-nucleus interactions,”
  Comput. Phys. Commun. 245, 106846 (2019), arXiv:1904.05129.

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Additional References for Alternative Models

If you utilize the optional alternative models included in the package, please also cite the respective source papers:

• Kamae et al. (2006) + Erratum:

  • T. Kamae, N. Karlsson, T. Mizuno, T. Abe, and T. Koi,
    “Parameterization of γ, e±, and Neutrino Spectra Produced by p-p Interaction in Astronomical Environments,”
    Astrophys. J. 647, 692–708 (2006), arXiv:astro-ph/0605581.
  • T. Kamae, N. Karlsson, T. Mizuno, T. Abe, and T. Koi,
    “Erratum: 'Parameterization of γ, e±, and Neutrino Spectra Produced by p-p Interaction in Astronomical Environments',”
    Astrophys. J. 662, 779 (2007).

• Kafexhiu et al. (2014):
  E. Kafexhiu, F. Aharonian, A. M. Taylor, and G. S. Vila,
  “Parametrization of gamma-ray production cross-sections for p-p interactions in a broad proton energy range from the kinematic threshold to PeV energies,”
  Phys. Rev. D 90, 123014 (2014), arXiv:1406.7369.