S(E)-Factor for (p,α) Induced Reactions on ^{11,10}B

Details S(E)-Factor for (p,α) Induced Reactions on ^{11,10}B S(E)-Factor for (p,α) Induced Reactions on ^{11,10}B

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374...73l&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Physics

Scientific paper

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 10^6 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 ^{11}B(p,α_0)^8Be and ^{10}B(p,α)^7Be reactions are reported.

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