Shell and explosive hydrogen burning
Nuclear Experiment
2016-11-30 v1
Abstract
The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized nuclides critically depend on the rates of the nuclear processes involved, often through non-trivial reaction chains, combined with complex mixing mechanisms. In this review, we summarize the contributions made by LUNA experiments in furthering our understanding of nuclear reaction rates necessary for modeling nucleosynthesis in AGB stars and Novae explosions.
Cite
@article{arxiv.1611.06244,
title = {Shell and explosive hydrogen burning},
author = {A. Boeltzig and C. G. Bruno and F. Cavanna and S. Cristallo and T. Davinson and R. Depalo and R. J. deBoer and A. Di Leva and F. Ferraro and G. Imbriani and P. Marigo and F. Terrasi and M. Wiescher},
journal= {arXiv preprint arXiv:1611.06244},
year = {2016}
}
Comments
23 pages, 12 figures