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| Paper: |
S(E)-Factor for (p,α) Induced Reactions on 11,10B |
| Volume: |
374, From Stars to Galaxies: Building the Pieces to Build Up the Universe |
| Page: |
73 |
| Authors: |
Lamia, L.; Pizzone, R.G.; Puglia, S.M.R.; Romano, S.; Carlin, N.; Cherubini, S.; Crucilla, V. |
| Abstract: |
Light elements lithium, beryllium and boron (LiBeB) seem to play a crucial role as probes for different mixing processes acting in stellar interior. Due to their fragility, these elements are mainly destroyed by (p,α) reactions occurring at temperatures of some 106 Kelvin. Detailed and precise informations about the S(E)-factor for such channels are then needed. To this aim, in this work the recent results about the 11B(p,α0)8Be and 10B(p,α)7Be reactions are reported. |
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