Abstract
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.
Original language | English |
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Pages (from-to) | 511-520 |
Number of pages | 10 |
Journal | Acta Physica Polonica B |
Volume | 44 |
Issue number | 3 |
DOIs | |
Publication status | Published - 1 Mar 2013 |
Externally published | Yes |