| Investigation of structure in 23Al via resonant proton scattering of 22Mg+p and the 22Mg(p,... |
| A Lorentzian-Function Approximation developed in calculating the charged-particle-induced n... |
| A revised 45V(p, g)46Cr astrophysical reaction rate |
| Single-particle resonance levels in 14O examined by 13N+p elastic resonance scattering |
| Search for signature inversion in the bands pi13/2？vi13/2 in 182,184,186Au |
| Signature inversion phenomena in odd-odd 182Au |
| Study of high-spin states in 143Pm |
| Synthesis and identification of a new heavy |
- 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
