The GALPROP program for cosmic-ray propagation: new developments
Astrophysics
2007-05-23 v1
Abstract
The cosmic-ray propagation code GALPROP has been generalized to include fragmentation networks of arbitrary complexity. The code can now provide an alternative to leaky-box calculations for full isotopic abundance calculations and has the advantage of including the spatial dimension which is essential for radioactive nuclei. Preliminary predictions for sub-Fe/Fe, 10Be/9Be, 26Al/27Al, 36Cl/Cl, and 54Mn/Mn are presented in anticipation of new experimental isotopic data.
Cite
@article{arxiv.astro-ph/9906228,
title = {The GALPROP program for cosmic-ray propagation: new developments},
author = {A. W. Strong and I. V. Moskalenko},
journal= {arXiv preprint arXiv:astro-ph/9906228},
year = {2007}
}
Comments
4 pages, 7 ps-figures, to appear in the Proceedings of 26th International Cosmic Ray Conference (Salt Lake City, 1999), OG 3.2.18 More details can be found at http://www.gamma.mpe-garching.mpg.de/~aws/aws.html