Light element evolution in the galactic halo

被引:0
|
作者
Alibès, A [1 ]
Canal, R [1 ]
机构
[1] Univ Barcelona, Dept Astron, E-08028 Barcelona, Spain
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:131 / 137
页数:7
相关论文
共 50 条