The experimental study of the astrophysical S-factor of 6Li(p, γ)7Be reaction
The low-energy astrophysical S-factors of the 6Li(p,γ)7Be reaction have been investigated on a new low energy experimental terminal which is designed for the low energy astrophysical experiments at the Institute of Modem Physics in Lanzhou.The S-factor of The experimental S-factor of this reaction shows an interesting sizable drop contrary to any existing theoretical expectations at energies below 200 keV.The structure of the S-factors hints a new level in 7Be.The spin and parity of this new level is discussed.In addition, our new results are discussed in the frame work ofa SUSY assisted Big-Bang Nucleosynthesis (BBN) model.
nuclear astrophysics cross-section S-factor Radiative capture
S.Z.Chen J.J.He S.W.Xu J.Hu C.E.Rolfs S.B.Ma S.Q.Hou X.Q.Yu M.Kusakabe T.Kajino
Institute of Modem Physics, Chinese Academy of Sciences, Lanzhou 730000, China;University of Chinese Institute of Modem Physics, Chinese Academy of Sciences, Lanzhou 730000, China Institute of Modem Physics, Chinese Academy of Sciences, Lanzhou 730000, China;Fakult(a)tfür Physiku Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan;Department of Astronomy, G
国际会议
昆明
英文
361-368
2014-05-01（万方平台首次上网日期，不代表论文的发表时间）