Study of the {sup 10}B(p,α){sup 7}Be reaction through the indirect Trojan Horse method
- INFN Laboratori Nazionali del Sud and CSFNM-Centrosiciliano Fisica Nucleare e Struttura della Materia,Catania (Italy)
- INFN Laboratori Nazionali del Sud and DMFCI- Università di Catania, Catania (Italy)
- Institute for Nuclear Physics, Prague-Rez (Czech Republic)
- Universidade de São Paulo - DFN, São Paulo (Brazil)
- China Institute of Atomic Energy, Beijing (China)
Boron abundances in stellar atmospheres, as well as berillium and lithium ones, can give useful hints for non-standard transport processes discrimination in stars. They can also be relevant for understanding several astrophysical processes (e.g. primordial nucleosynthesis and spallation reactions in ISM). A comprehensive study of Li Be B abundances can therefore confirm or not the presence of non-standard mixing processes in stellar envelopes. For this reason nuclear processes producing or depleting boron isotope abundance need to be studied at astrophysical energies. The {sup 10}B(p,α){sup 7}Be reaction has been studied by means of the Trojan Horse Method. The Trojan Horse Method was thus applied to the {sup 10}B(d,α{sup 7}Be)n reaction, studied at 24 MeV. The obtained results will be discussed.
- OSTI ID:
- 22391001
- Journal Information:
- AIP Conference Proceedings, Vol. 1645, Issue 1; Conference: Carpathian Summer School of Physics 2014, Sinaia (Romania), 13-26 Jul 2014; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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