| Issue |
EPJ Web of Conferences
Volume 66, 2014
INPC 2013 – International Nuclear Physics Conference
|
|
|---|---|---|
| Article Number | 07003 | |
| Number of page(s) | 4 | |
| Section | Nuclear Astrophysics | |
| DOI | https://doi.org/10.1051/epjconf/20146607003 | |
| Published online | 20 March 2014 | |
https://doi.org/10.1051/epjconf/20146607003
3He(α,γ)7Be cross section measured using complementary techniques
1 Instituto de Estructura de la Materia-CSIC, 28006-Madrid
2 TRIUMF, Vancouver, BC, Canada
3 Department of Physics, University of York, York, UK
4 Department of Particle Physics, Weizmann Institute of Science, Rehovot, Israel
a e-mail: m.carmona.gallardo@gmail.com
Published online: 20 March 2014
The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standard Model and in the Big Bang Nucleosynthesis scenario. The advances from two recent experiments performed using complementary techniques at center of mass (C.M.) energies between 1 and 3 MeV are discussed.
© Owned by the authors, published by EDP Sciences, 2014
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