Abstract: GALPROP is a numerical code for calculating the propagation of relativistic charged particles and the diffuse emissions produced during their propagation. The GALPROP code incorporates as much realistic astrophysical input as possible together with latest theoretical developments. The code calculates the propagation of cosmic-ray nuclei, antiprotons, electrons and positrons, and computes diffuse γ-rays and synchrotron emission in the same framework. Each run of the code is governed by a configuration file allowing the user to specify and control many details of the calculation. Thus, each run of the code corresponds to a potentially different "model." The code continues to be developed and is available to the scientific community.
Credit: Strong, A. W.; Moskalenko, I. V.; Porter, T. A.; Jóhannesson, G.; Orlando, E.; Digel, S. W.
Preferred citation method: Please see citation information here: https://galprop.stanford.edu/code.php?option=terms