We present the current status of the available data and the calculations for the cross section of the 3He(α, γ)7Be reaction — accurate knowledge of which is required for the solar neutrino flux and the primordial 7Li abundance calculations. Precision measurements are being carried out by us in the range of Ecm = 1 to 3 MeV using two types of experimental methods. A brief account of this work is given together with some of the recent theoretical calculations.
|Number of pages||10|
|Journal||Acta Physica Polonica B|
|Publication status||Published - 1 Mar 2013|