The GALPROP program for cosmic-ray propagation: new developments
| dc.creator | Strong, A. W. | |
| dc.creator | Moskalenko, I. V. | |
| dc.date | 1999-06-14 | |
| dc.date.accessioned | 2026-07-07T02:32:00Z | |
| dc.date.available | 2026-07-07T02:32:00Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9906228 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9906228 | |
| dc.identifier | Proc. 26th ICRC (Salt Lake City), 1999, v.4, p.255-258 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14360 | |
| dc.subject | Astrophysics | |
| dc.title | The GALPROP program for cosmic-ray propagation: new developments | |
| dc.type | text |