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NSR database version of April 11, 2024.

Search: Author = G.X.Li

Found 4 matches.

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2023WA16      Chin.Phys.C 47, 074103 (2023)

H.-K.Wang, A.Jalili, G.-X.Li, Y.-B.Wang

Monopole effects and high-spin levels in neutron-rich 132Te

NUCLEAR STRUCTURE 132Te; calculated energy levels, J, π using shell model calculations using the extended pairing plus multipole-multipole force model; deduced significant difference between experiment and theory in the high-spin level 17+, the monopole corrections and quadruple-quadruple force.

doi: 10.1088/1674-1137/accdc6
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2023ZH26      Phys.Rev. C 107, 065801 (2023)

H.Zhang, J.Su, Z.H.Li, Y.J.Li, E.T.Li, C.Chen, J.J.He, Y.P.Shen, G.Lian, B.Guo, X.Y.Li, L.Y.Zhang, Y.D.Sheng, Y.J.Chen, L.H.Wang, L.Zhang, F.Q.Cao, W.Nan, W.K.Nan, G.X.Li, N.Song, B.Q.Cui, L.H.Chen, R.G.Ma, Z.C.Zhang, T.Y.Jiao, B.S.Gao, X.D.Tang, Q.Wu, J.Q.Li, L.T.Sun, S.Wang, S.Q.Yan, J.H.Liao, Y.B.Wang, S.Zeng, D.Nan, Q.W.Fan, W.P.Liu

Updated reaction rate of 25Mg(p, γ)26Al and its astrophysical implication

NUCLEAR REACTIONS 25Mg(p, γ), E=117-350 keV; measured Eγ, Iγ, sum of γ energies; deduced γ-ray branching ratios, resonances, resonance strengths, astrophysical reaction rate (T=0.01-2.0 GK), contribution of individual resonances to the reaction rate, ground-state and isomeric state contribution. Comaprison to other experimental data and NACRE compilation. Evaluated the impact of the obtained data on the 26Al yield in stellar environment (code MESA). BGO detector array in nearby 4π geometry composed of 8 identical segments at high-current 400 kV JUNA accelerator (China JinPing underground Laboratory).

doi: 10.1103/PhysRevC.107.065801
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2022SO20      Astrophys.J. 941, 56 (2022)

N.Song, S.Zhang, Z.H.Li, G.X.Li, Z.C.Gao, H.K.Wang

Influence of Neutrino-Nuclear Reactions on the Abundance of 74Se

NUCLEAR REACTIONS 74Ge(ν, e-), E<60 MeV; calculated σ using experimental and theoretical B(GT).

doi: 10.3847/1538-4357/aca328
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2022WA41      Phys.Rev. C 106, 054316 (2022)

H.K.Wang, G.X.Li, B.Jiang, Y.B.Qian

Monopole effects and spin-trap structures in neutron-rich Te isotopes

NUCLEAR STRUCTURE 134,135,137,136,138,139Te; calculated levels, J, π, configurations. 134,135,136,138Te; calculated B(E2). Shell-model calculation using code NUSHELL with new Hamiltonian constructed with the intruder orbit νi13/2. Comparison to experimental data.

doi: 10.1103/PhysRevC.106.054316
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