1997/04/23 by Attila Csoto
Physics and Astronomy · #nucl-th #astro-ph
published as Heavy Ion Physics 6 (1997) 103 · 4 pages with 3 figures. To appear in the proceedings of the "Exotic Nuclear Shapes" Conference
arxiv created 1997/04/23 · arxiv updated 2009/12/01
The importance of the Be7(p,gamma)B8 reaction in predicting the high-energy solar neutrino flux is discussed. I present a microscopic eight-body model and a potential model for the calculation of the Be7(p,gamma)B8 cross section.