NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = G.X.Li Found 4 matches. 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
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
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
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
Back to query form |