Light Element Evolution in the Galactic Halo
Astrophysics
2007-05-23 v2
Abstract
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.
Cite
@article{arxiv.astro-ph/9901291,
title = {Light Element Evolution in the Galactic Halo},
author = {Andreu Alibes and Ramon Canal},
journal= {arXiv preprint arXiv:astro-ph/9901291},
year = {2007}
}
Comments
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)