Propagation of Light Elements in the Galaxy
| dc.creator | Moskalenko, I. V. | |
| dc.creator | Strong, A. W. | |
| dc.creator | Mashnik, S. G. | |
| dc.creator | Jones, F. C. | |
| dc.date | 2003-06-17 | |
| dc.date.accessioned | 2026-07-07T02:08:48Z | |
| dc.date.available | 2026-07-07T02:08:48Z | |
| dc.description | The origin and evolution of isotopes of the lightest elements H2, He3, Li, Be, B in the universe is a key problem in such fields as astrophysics of CR, Galactic evolution, non-thermal nucleosynthesis, and cosmological studies. One of the major sources of these species is spallation by CR nuclei in the interstellar medium. On the other hand, it is the B/C ratio in CR and Be10 abundance which are used to fix the propagation parameters and thus the spallation rate. We study the production and Galactic propagation of isotopes of elements Z<6 using the numerical propagation code GALPROP and updated production cross sections. | |
| dc.description | 4 pages, 6 ps-figures, tsukuba.sty, to appear in the Proc. 28th International Cosmic Ray Conference (Tsukuba, Japan 2003). More details can be found at http://www.gamma.mpe-garching.mpg.de/~aws/aws.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0306349 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0306349 | |
| dc.identifier | Proc. 28th ICRC Tsukuba, 2003, pp.1917-1920 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6198 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Propagation of Light Elements in the Galaxy | |
| dc.type | text |