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

Publisher: Edp Sciences

E-ISSN: 2100-014x|66|issue|07003-07003

ISSN: 2100-014x

Source: EPJ Web of Conference, Vol.66, Iss.issue, 2014-03, pp. : 07003-07003

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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.