Determination of the 3he(α, Γ)7be and 6li(p, Γ)7be Astrophysical Factors Down to Zero Energy Using the Asymptotic Normalization Coefficients
M. La Cognata,G. G. Kiss,R. Yarmukhamedov,K. I. Tursunmakhatov,I. Wiedenhover,L. T. Baby,S. Cherubini,A. Cvetinovic,G. D'Agata,P. Figuera,G. L. Guardo,M. Gulino,S. Hayakawa,I. Indelicato,L. Lamia,M. Lattuada,F. Mudo,S. Palmerini,R. G. Pizzone,G. G. Rapisarda,S. Romano,M. L. Sergi,R. Sparta,C. Spitaleri,O. Trippella,A. Tumino,M. Anastasiou,S. A. Kuvin,N. Rijal,B. Schmidt,S. B. Igamov,S. B. Sakuta,Zs. Fulop,Gy. Gyurky,T. Szucs,Z. Halasz,E. Somorjai,Z. Hons,J. Mrazek,R. E. Tribble,A. M. Mukhamedzhanov NUCLEAR PHYSICS IN ASTROPHYSICS - X, NPA-X 2022（2023）
Key words
Astrophysical Reaction Rates,Neutrino Detection
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