New advances for the 3He(4He,γ)7Be solar fusion reaction

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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 languageEnglish
Pages (from-to)511-520
Number of pages10
JournalActa Physica Polonica B
Volume44
Issue number3
DOIs
Publication statusPublished - 1 Mar 2013
Externally publishedYes

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