Abstract
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.
Original language | English |
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Article number | 07003 |
Number of pages | 4 |
Journal | EPJ Web of Conferences |
Volume | 66 |
DOIs | |
Publication status | Published - 20 Mar 2014 |