Determination of the ³He(α, γ)⁷Be and ⁶Li(p, γ)⁷Be astrophysical factors down to zero energy using the asymptotic normalization coefficients

The p - p -chain reaction 3 He( α , γ ) 7 Be can sensitively influence the prediction of the 7 Be and 8 B neutrino fluxes. Despite its importance, the knowledge of its reaction cross section at energies of the core of the Sun (15 keV 30 keV) is limited and the accuracy far from the desired 3% level. In the present paper the indirect measurement of the external capture contribution using the asymptotic normalization coefficient (ANC) technique is reported. The angular distributions of deuterons emitted in the 6 Li( 3 He, d ) 7 Be α -transfer reactions were measured and the ANCs extracted from the scaling of distorted-wave Born approximation (DWBA) and coupled-channel (CC) calculations. Then, the astrophysical S-factor for the 3 He( α , γ ) 7 Be reaction was calculated assuming E 1 direct capture and the zero energy value turned out to be 0.534 0.025 keVb. Both our experimental and theoretical approaches were benchmarked through the analysis of the 6 Li(p, γ ) 7 Be astrophysical factor, with interesting astrophysical applications to the understanding of the primordial lithium problem. In particular, the present work disfavors the occurrence of a claimed 200 keV resonance in the astrophysical factor.