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IMP Fulfils a Direct Reaction Cross-Section Measurement of 6Li(p,g)7Be at 320 kV Platform

Nuclear astrophysics strives for a comprehensive picture of the nuclear reactions responsible for synthesizing chemical elements and for powering the stellar evolution engine. Thereinto, the measurements of nuclear reaction cross sections (or expressed as S factors) at stellar Gamow energies are of great importance to nuclear astrophysics.

Researchers in Nuclear astrophysics group at the Institute of Modern Physics, Chinese Academy of Sciences (IMP) had established an experimental setup at the 320 kV platform in recent years. Based on this setup, the low-energy astrophysical S factors of the 6Li(p,g)7Be reaction were directly

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Group Leader: Prof.Jianjun HE
Address: Institute of Modern Physics, Chinese Academy of Sciences, 509 Nanchang Rd., Lanzhou
Post Code: 730000
Tel. 086-(0)931-4969312
E-mail: jianjunhe@impcas.ac.cn

Hign Energy Nuclear Physics Group