Abstract
We report on a new cross-section measurement for the He-3(alpha, gamma)(7) Be reaction at three medium energies of E-c.m. between 1 and 3 MeV. The interest stems from the significant role played by the reaction in calculating an accurate solar neutrino flux and the primordial Li-7 abundance. The energy dependence of the astrophysical S-34 factor observed in the present work, especially above 1 MeV, highlights the need to constrain theories in order to obtain a precise extrapolated value for S-34(0). In this context, a comparison with the recent theoretical work in a fully microscopic fermionic molecular dynamics approach and a few other representative calculations emphasize the need for further experimental as well as theoretical work to resolve the existing conflicts.
Original language | English |
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Article number | 032801 |
Pages (from-to) | 1-5 |
Number of pages | 5 |
Journal | Physical Review C |
Volume | 86 |
Issue number | 3 |
DOIs | |
Publication status | Published - 11 Sept 2012 |