Light Element Evolution in the Galactic Halo
| dc.creator | Alibes, Andreu | |
| dc.creator | Canal, Ramon | |
| dc.date | 1999-01-21 | |
| dc.date | 1999-02-24 | |
| dc.date.accessioned | 2026-07-07T02:30:07Z | |
| dc.date.available | 2026-07-07T02:30:07Z | |
| dc.description | Using a time-dependent Galactic Cosmic Ray flux proportional to the halo Star Formation Rate and including astration and neutrino-induced nucleosynthesis, we have studied the evolution of lithium, beryllium and boron in the halo. Our results set limits to the production of LiBeB by the neutrino-induced nucleosynthesis in massive stars, in order to reproduce the observed constancy of Be/Fe and B/Fe ratios, the lithium plateau and the isotopic ratios evolution. | |
| dc.description | latex 6 pages, 7 figures (Modified text content and figures). To appear in the Proceedings of the "Workshop on LiBeB, Cosmic Rays and Gamma-Ray Line Astronomy" (PASP) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9901291 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9901291 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13721 | |
| dc.subject | Astrophysics | |
| dc.title | Light Element Evolution in the Galactic Halo | |
| dc.type | text |