Astrophysical impact of the updated {sup 9}Be(p,α){sup 6}Li and {sup 10}B(p,α){sup 7}Be reaction rates as deduced by THM
- Department of Physics and Astronomy, University of Catania, Catania (Italy)
- INFN, Section of Pisa, Largo Bruno Pontecorvo 3, I-56127, Pisa (Italy)
- INFN—Laboratori Nazionali del Sud, Catania (Italy)
The complete understanding of the stellar abundances of lithium, beryllium, and boron represents one of the most interesting open problems in astrophysics. These elements are largely used to probe stellar structure and mixing phenomena in different astrophysical scenarios, such as pre-main-sequence or main-sequence stars. Their different fragility against (p,α) burning reactions allows one to investigate different depths of the stellar interior. Such fusion mechanisms are triggered at temperatures between T ≈ (2–5) × 10{sup 6} K, thus defining a corresponding Gamow energy between ≈ 3–10 keV, where S(E)-factor measurements need to be performed to get reliable reaction rate evaluations. The Trojan Horse Method is a well defined procedure to measure cross sections at Gamow energies overcoming the uncertainties due to low-energy S(E)-factor extrapolation as well as electron screening effects. Taking advantage of the THM measure of the {sup 9}Be(p,α){sup 6}Li and {sup 10}B(p,α){sup 7}Be cross sections, the corresponding reaction rates have been calculated and compared with the evaluations by the NACRE collaboration, widely used in the literature. The impact on surface abundances of the updated {sup 9}Be and {sup 10}B (p,α) burning rates is discussed for pre-MS stars.
- OSTI ID:
- 22882536
- Journal Information:
- Astrophysical Journal, Vol. 811, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X
- Country of Publication:
- United Kingdom
- Language:
- English
Similar Records
The AGB star nucleosynthesis in the light of the recent {sup 17}O(p,α){sup 14}N and {sup 18}O(p,α){sup 15}N reaction rate determinations
First Measurement of the {sup 19}F(α, p){sup 22}Ne Reaction at Energies of Astrophysical Relevance