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

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)


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
Issue number3
Publication statusPublished - 1 Mar 2013
Externally publishedYes


Dive into the research topics of 'New advances for the 3He(4He,γ)7Be solar fusion reaction'. Together they form a unique fingerprint.

Cite this