3He(α, γ)7Be cross section measured using complementary techniques

M. Carmona-Gallardo, A. Rojas, M. J G Borge, B. Davids, B. R. Fulton, M. Hass, B. S. Nara Singh, C. Ruiz, O. Tengblad

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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 languageEnglish
Article number07003
Number of pages4
JournalEPJ Web of Conferences
Publication statusPublished - 20 Mar 2014

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