NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = W.P.Liu Found 76 matches. 2023WA05 Phys.Rev.Lett. 130, 092701 (2023) L.H.Wang, J.Su, Y.P.Shen, J.J.He, M.Lugaro, B.Szanyi, A.I.Karakas, L.Y.Zhang, X.Y.Li, B.Guo, G.Lian, Z.H.Li, Y.B.Wang, L.H.Chen, B.Q.Cui, X.D.Tang, B.S.Gao, Q.Wu, L.T.Sun, S.Wang, Y.D.Sheng, Y.J.Chen, H.Zhang, Z.M.Li, L.Y.Song, X.Z.Jiang, W.Nan, W.K.Nan, L.Zhang, F.Q.Cao, T.Y.Jiao, L.H.Ru, J.P.Cheng, M.Wiescher, W.P.Liu Measurement of the 18O(α, γ)22Ne Reaction Rate at JUNA and Its Impact on Probing the Origin of SiC Grains NUCLEAR REACTIONS 18O(α, γ), E=470-787 keV; measured reaction products, Eγ, Iγ; deduced thick target yields, resonance energies and resonance strengths, total reaction rates. Comparison with available data. The Jinping Underground Nuclear Astrophysics experimental facility (JUNA).
doi: 10.1103/PhysRevLett.130.092701
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
2022AL01 J.Phys.(London) G49, 010501 (2022) M.Aliotta, R.Buompane, M.Couder, A.Couture, R.J.deBoer, A.Formicola, L.Gialanella, J.Glorius, G.Imbriani, M.Junker, C.Langer, A.Lennarz, Y.A.Litvinov, W.-P.Liu, M.Lugaro, C.Matei, Z.Meisel, L.Piersanti, R.Reifarth, D.Robertson, A.Simon, O.Straniero, A.Tumino, M.Wiescher, Y.Xu The status and future of direct nuclear reaction measurements for stellar burning NUCLEAR REACTIONS 12C(α, γ), 22Ne(α, n), (α, γ), 12C(12C, X), E(cm)<7 MeV; analyzed available data; deduced σ, S-factors.
doi: 10.1088/1361-6471/ac2b0f
2022LI28 Few-Body Systems 63, 43 (2022) W.P.Liu, Z.H.Li, J.J.He, X.D.Tang, G.Lian, J.Su, Y.P.Shen, Z.An, F.Q.Chao, J.J.Chang, L.H.Chen, H.Chen, X.J.Chen, Y.H.Chen, Z.J.Chen, B.Q.Cui, X.C.Du, X.Fang, C.B.Fu, L.Gan, B.Guo, Z.Y.Han, X.Y.Guo, G.Z.He, J.R.He, A.Heger, S.Q.Hou, H.X.Huang, N.Huang, B.L.Jia, L.Y.Jiang, S.Kubono, J.M.Li, M.C.Li, K.A.Li, E.T.Li, T.Li, Y.J.Li, M.Lugaro, X.B.Luo, H.Y.Ma, S.B.Ma, D.M.Mei, W.Nan, W.K.Nan, N.C.Qi, Y.Z.Qian, J.C.Qin, J.Ren, C.S.Shang, L.T.Sun, W.L.Sun, W.P.Tan, I.Tanihata, S.Wang, P.Wang, Y.B.Wang, Q.Wu, S.W.Xu, S.Q.Yan, L.T.Yang, Y.Yang, X.Q.Yu, Q.Yue, S.Zeng, L.Zhang, H.Zhang, H.Y.Zhang, L.Y.Zhang, N.T.Zhang, P.Zhang, Q.W.Zhang, T.Zhang, X.P.Zhang, X.Z.Zhang, W.Zhao, J.F.Zhou, Y.Zho Progress of Underground Nuclear Astrophysics Experiment JUNA in China NUCLEAR REACTIONS 12C(α, γ), 13C(α, n), 25Mg(p, γ), 19F(p, α), E(cm)<600 keV; measured reaction products; deduced yields near the Gamow window. Comparison with available data.
doi: 10.1007/s00601-022-01735-3
2022LI47 Phys.Rev. C 106, 025807 (2022) X.Y.Li, B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, J.J.He, S.Q.Yan, Q.W.Fan, J.C.Liu, L.Gan, Z.Y.Han, E.T.Li, G.Lian, Y.P.Shen, Y.B.Wang, S.Zeng, W.P.Liu Astrophysical 15N(n, γ)16N reaction rate from precision measurement of the 15N(d, p)16N angular distributions NUCLEAR REACTIONS 15N(d, p), (d, d), E=15 MeV; measured particle spectra, σ(θ) using Q3D magnetic spectrograph at CIAE's HI-13 tandem accelerator facility. 16N; deduced levels, J, π, configurations, spectroscopic factors for ground and first three excited states. DWBA and ADWA analysis. 15N(n, γ), T=0.01-10 GK; deduced astrophysical reaction rates; calculated σ(E). Comparison with previous experimental results, and with OXBASH shell-model predictions.
doi: 10.1103/PhysRevC.106.025807
2022WA02 Nucl.Instrum.Methods Phys.Res. B512, 49 (2022) L.H.Wang, Y.P.Shen, J.Su, X.Y.Li, W.Q.Yan, J.J.He, L.Y.Zhang, B.Liao, Y.F.Wu, Y.D.Sheng, Z.M.Li, Y.J.Chen, L.Y.Song, X.Z.Jiang, G.Lian, W.Nan, W.K.Nan, L.Zhang, F.Q.Cao, C.Chen, N.Song, H.Zhang, W.P.Liu Development of irradiation-resistant enriched 12C targets for astrophysical 12C(α, γ)16O reaction measurements NUCLEAR REACTIONS 12C(p, γ), E=370 keV; 12C(p, α), E=740 keV; measured reaction products, Eγ, Iγ; deduced yields. The China JinPing underground Laboratory (CJPL).
doi: 10.1016/j.nimb.2021.11.020
2022ZH67 Phys.Rev. C 106, 055803 (2022) L.Y.Zhang, J.Su, J.J.He, R.J.deBoer, D.Kahl, M.Wiescher, D.Odell, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, B.Guo, X.D.Tang, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, J.P.Cheng, W.P.Liu Direct measurement of the astrophysical 19F(p, αγ)16O reaction in a deep-underground laboratory NUCLEAR REACTIONS 19F(p, αγ), E(cm)=72.4-344 keV; measured Eγ, Iγ; deduced astrophysical S-factor, thermonuclear astrophysical reaction rates (range 0.05–1 GK), contributions from different channels. R-matrix analysis with AZURE2 together with a MCMC Bayesian uncertainty estimation. Comparison to other experimental data. 4π BGO γ-array with proton beam from JUNA accelerator at China JinPing underground Laboratory (CJPL).
doi: 10.1103/PhysRevC.106.055803
2021ZH46 Chin.Phys.C 48, 084108 (2021) H.Zhang, Z.i-H.Li, J.Su, Y.-J.Li, C.Chen, L.Zhang, F.-Q.Cao, Y.-P.Shen, W.Nan, W.-K.Nan, X.-Y.Li, L.-H.Chen, G.Lian, B.-Q.Cui, B.Guo, W.-P.Liu Direct measurement of the resonance strengths and branching ratios of low-energy (p, γ) reactions on Mg isotopes NUCLEAR REACTIONS 24,25,26Mg(p, γ), E=220-400 keV; measured reaction products, Eγ, Iγ; deduced γ-ray energies, yields, resonances, branching ratios, resonance strengths. JUNA experiment, comparison with NACRE data.
doi: 10.1088/1674-1137/ac06aa
2021ZH53 Phys.Rev.Lett. 127, 152702 (2021) L.Y.Zhang, J.Su, J.J.He, M.Wiescher, R.J.deBoer, D.Kahl, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, X.D.Tang, H.W.Zhao, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, B.Guo, S.W.Xu, J.Y.Li, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, X.H.Zhou, Y.H.Zhang, F.S.Zhang, Z.G.Hu, H.S.Xu, J.P.Chen, W.P.Liu Direct Measurement of the Astrophysical 19F(p, αγ)16O Reaction in the Deepest Operational Underground Laboratory NUCLEAR REACTIONS 19F(p, α), E(cm)=72.4-188.8 keV; measured reaction products, Eγ, Iγ; deduced yields, S-factors, reaction rates. The China Jinping Underground Laboratory (CJPL), JUNA accelerator.
doi: 10.1103/physrevlett.127.152702
2020GA03 Phys.Rev. C 101, 014612 (2020) L.Gan, H.B.Sun, Z.H.Li, S.P.Hu, Y.J.Li, J.Su, B.Guo, S.Q.Yan, Y.B.Wang, S.Zeng, Z.Y.Han, X.Y.Li, D.H.Li, T.L.Ma, Y.P.Shen, Y.Su, E.T.Li, W.P.Liu Experimental study of the spectroscopic factors of 116-125Sn NUCLEAR REACTIONS 116,118,120,122,124Sn(p, d), E=18.0 MeV; 116,118,120,122,124Sn(d, p), E=12.0 MeV; measured E(p), I(p), E(d), I(d), σ(θ) using the high-precision Q3D magnetic spectrograph at the CIAE-Beijing HI-13 tandem accelerator. 115,117,119,121,123,125Sn; deduced levels, L-transfers, J, π, spectroscopic factors (SFs). DWBA analysis of σ(θ) data and extraction of the neutron spectroscopic factors using two different sets of systematic optical potential parameters. Comparison with previous experimental data. Proposed a linear formula to relate SFs with S(n).
doi: 10.1103/PhysRevC.101.014612
2020LI17 Chin.Phys.C 44, 074001 (2020) X.-Y.Li, B.Guo, Z.-H.Li, W.-P.Liu Astrophysical 22Mg(p, γ)23Al reaction rates from asymptotic normalization coefficient of 23Ne → 22Ne + n RADIOACTIVITY 23Ne(n); analyzed available data; calculated squared neutron asymptotic normalization coefficients (ANCs) from the experimental differential cross-sections of the 22Ne(d, p) reaction through the ADWA and CDCC analysis.
doi: 10.1088/1674-1137/44/7/074001
2020LI31 Phys.Rev. C 102, 025804 (2020) Y.J.Li, Z.H.Li, E.T.Li, X.Y.Li, T.L.Ma, Y.P.Shen, J.C.Liu, L.Gan, Y.Su, L.H.Qiao, Z.Y.Han, Y.Zhou, J.Su, S.Q.Yan, S.Zeng, Y.B.Wang, B.Guo, G.Lian, D.Nan, X.X.Bai, W.P.Liu Indirect measurement of the 57.7 keV resonance strength for the astrophysical γ-ray source of the 25Mg(p, γ)26Al reaction NUCLEAR REACTIONS 24,25Mg(7Li, 6He), (7Li, 7Li), E=31.5 MeV; measured 6He and 7Li particle spectra using ΔE-E telescope of Si detectors, σ(θ) using Q3D magnetic spectrometer at the HI-13 tandem accelerator of CIAE-Beijing. 26Al; deduced levels, J, π, spectroscopic factors. DWBA analysis of σ(θ) data using the code FRESCO, with Woods-Saxon potential parameters deduced from analysis of the present data and the literature data for 27Al(6Li, 6Li) reaction. 25Mg(p, γ)26Al; deduced Γp and resonance strength of 57.7-keV proton resonance in 26Al. 25Mg(p, γ)26Al, T9=0.1-10; calculated astrophysical reaction rates for the ground and isomeric states in 26Al, and compared with the results in the NACRE database.
doi: 10.1103/PhysRevC.102.025804
2020RO16 Chin.Phys.C 44, 104003 (2020) C.-H.Rong, G.-L.Zhang, L.Gan, Z.-Ho.Li, L.C.Brandao, E.N.Cardozo, M.R.Cortes, Y.-J.Li, Ju.Su, S.-Q.Yan, S.Zeng, G.Lian, B.Guo, Y.-B.Wang, W.-P.Liu, J.Lubian The angular distributions of elastic scattering of 12, 13C+Zr NUCLEAR REACTIONS 90,91,92,94,96Zr(12C, 12C), (13C, 13C), E=66, 64 MeV; measured reaction products; deduced σ, the neutron spectroscopic amplitudes using the optical model and coupled channel calculations.
doi: 10.1088/1674-1137/abab8d
2020SH09 Phys.Rev.Lett. 124, 162701 (2020) Y.P.Shen, B.Guo, R.J.deBoer, Z.H.Li, Y.J.Li, X.D.Tang, D.Y.Pang, S.Adhikari, C.Basu, J.Su, S.Q.Yan, Q.W.Fan, J.C.Liu, C.Chen, Z.Y.Han, X.Y.Li, G.Lian, T.L.Ma, W.Nan, W.K.Nan, Y.B.Wang, S.Zeng, H.Zhang, W.P.Liu Constraining the External Capture to the 16O ground State and the E2 S Factor of the 12C(α, γ)16O reaction NUCLEAR REACTIONS 12C(11B, 7Li)16O, E=50 MeV; measured reaction products; deduced σ(θ), the ground state asymptotic normalization coefficients, S-factors. Comparison with available data.
doi: 10.1103/PhysRevLett.124.162701
2019MA31 Nucl.Phys. A986, 26 (2019) T.L.Ma, B.Guo, Z.H.Li, Y.J.Li, D.Y.Pang, Y.L.Han, Y.P.Shen, J.Su, J.C.Liu, Q.W.Fan, Z.Y.Han, X.Y.Li, G.Lian, Y.Su, Y.B.Wang, S.Q.Yan, S.Zeng, W.P.Liu Precision measurement of the angular distribution for the 16O(d, p)17O transfer reaction to the ground state of 17O NUCLEAR REACTIONS 16O(d, p)17O, E=15 MeV; measured Ep, Ip(θ); deduced σ(θ) for reactions to 17O gs, spectroscopic factors, ANC; calculated σ(θ) for reactions to 17O gs using DWBA, ADWA (Adiabatic DWBA) and Continuum Discretized Coupled Channel (CDCC) vs radius parameter of Woods-Saxon potential with the same optical potential parameters in ADWA and CDCC. SF and ANC for 17O compared with published results in heavy ion transfer and with shell model calculations.
doi: 10.1016/j.nuclphysa.2019.03.004
2019SH11 Phys.Rev. C 99, 025805 (2019) Y.P.Shen, B.Guo, Z.H.Li, Y.J.Li, D.Y.Pang, S.Adhikari, Z.D.An, J.Su, S.Q.Yan, X.C.Du, Q.W.Fan, L.Gan, Z.Y.Han, D.H.Li, E.T.Li, X.Y.Li, G.Lian, J.C.Liu, T.L.Ma, C.J.Pei, Y.Su, Y.B.Wang, S.Zeng, Y.Zhou, W.P.Liu Astrophysical SE2 factor of the 12C (α, γ)16O reaction through the 12C(11B, 7Li)16O transfer reaction NUCLEAR REACTIONS 12C(11B, 7Li), (11B, 11B), E=50 MeV; 16O(7Li, 7Li), E=26 MeV; measured charged-particle spectra, differential σ(θ) using the Q3D magnetic spectrograph at the HI-13 tandem accelerator of the CIAE-Beijing. 12C(α, γ), E(cm)<5 MeV; deduced astrophysical SE2(300) factor of the ground state. 16O; deduced asymptotic normalization coefficient (ANC) and reduced α width of the 6.917-MeV level from finite-range distorted wave Born approximation (FRDWBA) and coupled-reaction-channel (CRC) analysis using FRESCO code. Comparison with previous experimental values, and with theoretical model predictions. R-matrix analysis of scattering data.
doi: 10.1103/PhysRevC.99.025805
2019SH37 Phys.Lett. B 797, 134820 (2019) Y.P.Shen, B.Guo, T.L.Ma, D.Y.Pang, D.D.Ni, Z.Z.Ren, Y.J.Li, Z.D.An, J.Su, J.C.Liu, Q.W.Fan, Z.Y.Han, X.Y.Li, Z.H.Li, G.Lian, Y.Su, Y.B.Wang, S.Q.Yan, S.Zeng, W.P.Liu First experimental constraint of the spectroscopic amplitudes for the α-cluster in the 11B ground state NUCLEAR REACTIONS 7Li(6Li, d), E=24 MeV; measured reaction products; deduced spectroscopic amplitudes (SA) for the α-cluster in the 11B ground state. Comparison with available data.
doi: 10.1016/j.physletb.2019.134820
2018GA19 Phys.Rev. C 97, 064614 (2018) L.Gan, H.B.Sun, Z.H.Li, Y.J.Li, J.Su, B.Guo, S.Q.Yan, Y.B.Wang, S.Zeng, Z.Y.Han, X.Y.Li, D.H.Li, T.L.Ma, Y.P.Shen, Y.Su, E.T.Li, S.P.Hu, W.P.Liu Experimental study of the spectroscopic factors of 90-97Zr NUCLEAR REACTIONS 90,92,94,96Zr(12C, 12C), (12C, 13C), E=66 MeV; 90,92,94,96Zr(13C, 13C), (13C, 12C), E=64 MeV; measured particle spectra, differential σ(θ) using Q3D magnetic spectrograph at the HI-13 tandem accelerator facility of the CIAE, Beijing; deduced neutron spectroscopic factors using distorted-wave Born approximation (DWBA) calculations. Comparison of spectroscopic results with previous experiments. Relevance to neutron capture reactions in s process for synthesis of heavy elements.
doi: 10.1103/PhysRevC.97.064614
2018HE01 Chin.Phys.C 42, 015001 (2018) J.-J.He, I.Lombardo, D.Dell'Aquila, Y.Xu, L.-Y.Zhang, W.-P.Liu Thermonuclear 19F(p, α0)16O reaction rate NUCLEAR REACTIONS 19F(p, α), E<1 MeV; analyzed available data; deduced reaction rate, σ, σ(θ), S-factor using theoretical R-matrix extrapolations.
doi: 10.1088/1674-1137/42/1/015001
2018LI18 Chin.Phys.C 42, 044001 (2018) E.-T.Li, Z.H.Li, S.-Q.Yan, J.Su, B.Guo, Y.-J.Li, Y.-B.Wang, G.Lian, S.Zeng, S.-Z.Chen, S.-B.Ma, X.-Q.Li, C.He, H.-B.Sun, W.-P.Liu Measurement of the 2H(7Be, 6Li)3He reaction rate and its contribution to the primordial lithium abundance NUCLEAR REACTIONS 2H(7Be, 6Li)3He, E=17.7, 30.2 MeV; measured reaction products, Eα, Iα; deduced σ(θ), σ, reaction rates. Comparison with theoretical calculations.
doi: 10.1088/1674-1137/42/4/044001
2018LI24 Chin.Phys.C 42, 065001 (2018) Z.-H.Li, E.-T.Li, J.Su, Y.-J.Li, Y.-B.Wang, S.-Q.Yan, B.Guo, D.Nan, W.-P.Liu New determination of the 7Be ground state spectroscopic factor and the 6Li(p, γ)7Be astrophysical S(E)factors NUCLEAR REACTIONS 7Be(d, 3He)6Li, E(cm)=6.7 MeV; measured reaction products; deduced σ(θ). 6Li(p, γ)7Be, E(cm)<1 MeV; analyzed available data; deduced S factors. Comparison with DWBA calculation code TWOFNR.
doi: 10.1088/1674-1137/42/6/065001
2017QU08 Phys.Rev. C 96, 054309 (2017) S.Quan, W.P.Liu, Z.P.Li, M.S.Smith Microscopic core-quasiparticle coupling model for spectroscopy of odd-mass nuclei NUCLEAR STRUCTURE 224Ra, 144,146,148,150,152,154Ba; calculated free energy surface contours in (β2, β3) plane, global minima deformations β2, β3, β4, excitation energies, pairing gaps, specific heat, neutron and proton single-particle levels as a function of temperature. Finite-temperature deformed RMF+BCS theory based on the relativistic point-coupling density functional.
doi: 10.1103/PhysRevC.96.054309
2017YA27 Astrophys.J. 848, 98 (2017) S.Q.Yan, Z.H.Li, Y.B.Wang, K.Nishio, M.Lugaro, A.I.Karakas, H.Makii, P.Mohr, J.Su, Y.J.Li, I.Nishinaka, K.Hirose, Y.L.Han, R.Orlandi, Y.P.Shen, B.Guo, S.Zeng, G.Lian, Y.S.Chen, W.P.Liu The 95Zr(n, γ)96Zr Cross Section from the Surrogate Ratio Method and Its Effect on s-process Nucleosynthesis NUCLEAR REACTIONS 94,90Zr(18O, 16O), E=117 MeV; measured reaction products; deduced σ for surrogate reactions. Comparison with KADONIS and ENDF/B-VII.1 evaluated nuclear library and TALYS nuclear code calculations.
doi: 10.3847/1538-4357/aa8c74
2016LI18 Sci.China: Phys.Mech.Astron. 59, 642001 (2016) W.P.Liu, for the JUNA Collaboration Progress of Jinping Underground laboratory for Nuclear Astrophysics (JUNA)
doi: 10.1007/s11433-016-5785-9
2016LI51 Chin.Phys.C 40, 114104 (2016) E.T.Li, B.Guo, Z.H.Li, Y.B.Wang, Y.J.Li, Z.D.Wu, J.Su, D.Y.Pang, X.X.Bai, X.C.Du, Q.W.Fan, L.Gan, Z.Y.Han, X.Hao, S.P.Hu, J.J.He, L.Jing, S.J.Jin, L.Li, X.Y.Li, Z.C.Li, G.Lian, J.C.Liu, Q.Luo, L.H.Qiao, Y.P.Shen, H.B.Sun, S.Q.Yan, X.Q.Yu, S.Zeng, D.H.Zhang, L.Y.Zhang, W.J.Zhang, Y.Zhou, W.P.Liu Radii of the bound states in 16N from the asymptotic normalization coefficients RADIOACTIVITY 16N(n) [from 15N(7Li, 6Li)16N, E=44 MeV]; analyzed available data; deduced asymptotic normalization coefficients (ANCs), rms radii of the valence neutron, probabilities of the valence neutron staying out of the core potentials.
doi: 10.1088/1674-1137/40/11/114104
2016SU10 Phys.Lett. B 756, 323 (2016) J.Su, W.P.Liu, N.T.Zhang, Y.P.Shen, Y.H.Lam, N.A.Smirnova, M.MacCormick, J.S.Wang, L.Jing, Z.H.Li, Y.B.Wang, B.Guo, S.Q.Yan, Y.J.Li, S.Zeng, G.Lian, X.C.Du, L.Gan, X.X.Bai, Z.C.Gao, Y.H.Zhang, X.H.Zhou, X.D.Tang, J.J.He, Y.Y.Yang, S.L.Jin, P.Ma, J.B.Ma, M.R.Huang, Z.Bai, Y.J.Zhou, W.H.Ma, J.Hu, S.W.Xu, S.B.Ma, S.Z.Chen, L.Y.Zhang, B.Ding, Z.H.Li, G.Audi Revalidation of the isobaric multiplet mass equation at A = 53, T = 3/2 RADIOACTIVITY 53Ni(EC), (ECp) [from Be(58Ni, X)53Ni, E=68.3 MeV/nucleon]; measured decay products, Eγ, Iγ; deduced T1/2, level scheme, J, π, isobaric analog state, mass excess, explanation of unexpected deviation from the isobaric multiplet mass equation (IMME) at A=53, T=3/2.
doi: 10.1016/j.physletb.2016.03.024
2016YA09 Phys.Rev. C 94, 015804 (2016) S.Q.Yan, Z.H.Li, Y.B.Wang, K.Nishio, H.Makii, J.Su, Y.J.Li, I.Nishinaka, K.Hirose, Y.L.Han, R.Orlandi, Y.P.Shen, B.Guo, S.Zeng, G.Lian, Y.S.Chen, X.X.Bai, L.H.Qiao, W.P.Liu Examination of the surrogate ratio method for the determination of the 93Zr (n, γ)94Zr cross section with 90, 92Zr(18O, 16O) 92, 94Zr reactions NUCLEAR REACTIONS 90,92Zr(18O, 16O), E=117 MeV; measured Eγ, Iγ, (16O)γ-coin at the Tandem accelerator of JAEA facility. 92,94Zr; measured γ-decay probability ratios. 93Zr(n, γ), E>3 MeV; deduced σ(E) by surrogate ratio method, using reference cross sections of the 91Zr(n, γ)92Zr reaction from ENDF/B-VII.1, and the measured γ-decay probability ratios.
doi: 10.1103/PhysRevC.94.015804
2015KI07 Phys.Rev. C 92, 035801 (2015) A.Kim, N.H.Lee, M.H.Han, J.S.Yoo, K.I.Hahn, H.Yamaguchi, D.N.Binh, T.Hashimoto, S.Hayakawa, D.Kahl, T.Kawabata, Y.Kurihara, Y.Wakabayashi, S.Kubono, S.Choi, Y.K.Kwon, J.Y.Moon, H.S.Jung, C.S.Lee, T.Teranishi, S.Kato, T.Komatsubara, B.Guo, W.P.Liu, B.Wang, Y.Wang Measurement of the 14O(α, p)17F cross section at Ec.m. ≈ 2.1-5.3MeV NUCLEAR REACTIONS 4He(14O, p), E=2.5 MeV/nucleon, [secondary 14O beam from 1H(14N, n), E=8.4 MeV/nucleon primary reaction at RIBF-RIKEN]; measured E(p), I(p), pp-coin, energy distribution of single- and double-proton events, differential cross sections by thick target method. 18Ne; deduced levels, resonances, J, π, proton and α widths by R-matrix analysis, astrophysical reaction rates, strong single-proton decay events, but no strong double-proton events. Relevance to trigger reaction for the x-ray burst and nucleosynthesis of heavy nuclei up to Cd.
doi: 10.1103/PhysRevC.92.035801
2015SH16 Phys.Rev. C 91, 047304 (2015) Y.P.Shen, W.P.Liu, J.Su, N.T.Zhang, L.Jing, Z.H.Li, Y.B.Wang, B.Guo, S.Q.Yan, Y.J.Li, S.Zeng, G.Lian, X.C.Du, L.Gan, X.X.Bai, J.S.Wang, Y.H.Zhang, X.H.Zhou, X.D.Tang, J.J.He, Y.Y.Yang, S.L.Jin, P.Ma, J.B.Ma, M.R.Huang, Z.Bai, Y.J.Zhou, W.H.Ma, J.Hu, S.W.Xu, S.B.Ma, S.Z.Chen, L.Y.Zhang, B.Ding, Z.H.Li Measurement of the 52Fe mass via the precise proton-decay energy of 53Com RADIOACTIVITY 53mCo(p)[from 9Be(58Ni, X), E=68.3 MeV/nucleon]; 41Ti(β+p); measured Ep, Ip, at RIBLL-HIRFL-Lanzhou facility; deduced mass excess of 52Fe and compared with AME-2012 evaluation. 51Fe, 52Co(β+); measured half-lives and compared with evaluated data in ENSDF. ATOMIC MASSES 52Fe; deduced mass excess from Q value of proton decay of 3174.1 keV, 19/2- isomer in 53Co determined from measured proton energy. Comparison with previous experimental results.
doi: 10.1103/PhysRevC.91.047304
2014GU02 Phys.Rev. C 89, 012801 (2014) B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, S.Q.Yan, Z.D.Wu, E.T.Li, X.X.Bai, X.C.Du, Q.W.Fan, L.Gan, J.J.He, S.J.Jin, L.Jing, L.Li, Z.C.Li, G.Lian, J.C.Liu, Y.P.Shen, Y.B.Wang, X.Q.Yu, S.Zeng, L.Y.Zhang, W.J.Zhang, W.P.Liu Spectroscopic factors for low-lying 16N levels and the astrophysical 15N(n, γ)16N NUCLEAR REACTIONS 15N(7Li, 6Li)16N, E=44 MeV; measured 6Li spectrum, σ(θ) using Q3D magnetic spectrograph at CIAE's HI-13 tandem accelerator facility. 16N; deduced levels, J, π, configurations, spectroscopic factors for ground and first three excited states. DWBA analysis. Comparison with shell model calculations. 15N(n, γ)16N, at T=0.01-3 GK; deduced astrophysical reaction rates. Comparison with previous experimental and theoretical results.
doi: 10.1103/PhysRevC.89.012801
2014LI49 Phys.Rev. C 90, 067601 (2014) E.T.Li, Z.H.Li, Y.J.Li, B.Guo, Y.B.Wang, D.Y.Pang, J.Su, S.Q.Yan, S.Zeng, L.Gan, Z.C.Li, J.C.Liu, X.X.Bai, Z.D.Wu, S.J.Jin, L.Y.Zhang, X.Q.Yu, L.Li, H.B.Sun, G.Lian, Q.W.Fan, W.P.Liu Proton spectroscopic factor of the 12C ground state from the 12C(11B, 12C) 11B elastic transfer reaction NUCLEAR REACTIONS 12C(11B, 11B), (11B, 12C)11B, E=50 MeV; measured particle spectra, angular distributions using Q3D magnetic spectrometer at the HI-13 tandem accelerator of CIAE facility. 12C; deduced optical potential parameters, proton spectroscopic factor for 12C g.s., DWBA calculations. Comparison with previous experimental and theoretical results.
doi: 10.1103/PhysRevC.90.067601
2014WU03 Phys.Rev. C 89, 054315 (2014) Z.D.Wu, B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, S.Q.Yan, E.T.Li, X.X.Bai, X.C.Du, Q.W.Fan, L.Gan, J.J.He, S.J.Jin, L.Jing, L.Li, Z.C.Li, G.Lian, J.C.Liu, Y.P.Shen, Y.B.Wang, X.Q.Yu, S.Zeng, D.H.Zhang, L.Y.Zhang, W.J.Zhang, W.P.Liu Proton widths of the low-lying 16F states from the 15N(7Li, 6Li)16N reaction NUCLEAR REACTIONS 15N(7Li, 7Li), (7Li, 6Li), E=34.5, 44 MeV; measured particle spectra, elastic and inelastic σ(θ) using Q3D magnetic spectrograph at CIAE facility. 16N; deduced levels, J, π, asymptotic normalization coefficients (ANCs), spectroscopic factors. DWBA analysis. 16F; deduced proton and single-particle widths, spectroscopic factors for first four levels from mirror analogy with 16N. Comparison with previous experimental results and compilation.
doi: 10.1103/PhysRevC.89.054315
2013FA10 Phys.Rev. C 88, 045801 (2013) J.Fallis, A.Parikh, P.F.Bertone, S.Bishop, L.Buchmann, A.A.Chen, G.Christian, J.A.Clark, J.M.D'Auria, B.Davids, C.M.Deibel, B.R.Fulton, U.Greife, B.Guo, U.Hager, C.Herlitzius, D.A.Hutcheon, J.Jose, A.M.Laird, E.T.Li, Z.H.Li, G.Lian, W.P.Liu, L.Martin, K.Nelson, D.Ottewell, P.D.Parker, S.Reeve, A.Rojas, C.Ruiz, K.Setoodehnia, S.Sjue, C.Vockenhuber, Y.B.Wang, C.Wrede Constraining nova observables: Direct measurements of resonance strengths in 33S(p, γ)34Cl NUCLEAR REACTIONS 1H(33S, γ)34Cl, E=194-514 MeV/nucleon; measured particle spectra, time-of-flight using DRAGON at ISAC-TRIUMF facility. 34Cl; deduced levels, resonances, resonance strengths, thermonuclear reaction rates for 33S(p, γ)34Cl reaction at T9=0.15-0.40, composition of 32,33,34S, 35,37Cl, 36,38Ar, 38,39K, 40Ca in oxygen-neon nova ejecta. Implications for nova nucleosynthesis.
doi: 10.1103/PhysRevC.88.045801
2013GU04 Phys.Rev. C 87, 015803 (2013) B.Guo, J.Su, Z.H.Li, Y.B.Wang, S.Q.Yan, Y.J.Li, N.C.Shu, Y.L.Han, X.X.Bai, Y.S.Chen, W.P.Liu, H.Yamaguchi, D.N.Binh, T.Hashimoto, S.Hayakawa, D.Kahl, S.Kubono, J.J.He, J.Hu, S.W.Xu, N.Iwasa, N.Kume, Z.H.Li Determination of the astrophysical 12N(p, γ)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications NUCLEAR REACTIONS 2H(12N, 13O)1n, E=59 MeV; measured reaction products, energy loss, time-of-flight, differential σ(θ); deduced ANC, astrophysical S factors. 12N(p, γ)13O, at T9=0.3-3.0; deduced stellar reaction rate. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.87.015803
2013JI13 Phys.Rev. C 88, 035801 (2013) S.J.Jin, Y.B.Wang, J.Su, S.Q.Yan, Y.J.Li, B.Guo, Z.H.Li, S.Zeng, G.Lian, X.X.Bai, W.P.Liu, H.Yamaguchi, S.Kubono, J.Hu, D.Kahl, H.S.Jung, J.Y.Moon, C.S.Lee, T.Teranishi, H.W.Wang, H.Ishiyama, N.Iwasa, T.Komatsubara, B.A.Brown Resonant scattering of 22Na+p studied by the thick-target inverse-kinematic method NUCLEAR REACTIONS 1H(22Na, 22Na), E<37.1 MeV, [22Na secondary beam from 1H(22Ne, 22Na), E=6.0 MeV/nucleon primary reaction]; measured back-angle recoil-proton spectra, TOF, differential σ(E) using thick target technique at RIBF-RIKEN facility. R-matrix analysis of resonance spectra. 23Mg; deduced levels, resonances, J, π, Γp, Γγ, resonance strengths, two s-wave resonances. Comparison with previous experimental data, and with shell-model calculations. 22Na(p, γ)23Mg, T9=0.01-10; deduced astrophysical reaction rates. Comparison with previous experimental data and NACRE evaluation. NUCLEAR STRUCTURE 23Mg; calculated levels, J, π, s-wave resonances, their spectroscopic factors and γ widths using shell model with usda and usdb interactions. Comparison with experimental data, and with structure of 23Na mirror nucleus.
doi: 10.1103/PhysRevC.88.035801
2013LI09 Phys.Rev. C 87, 017601 (2013) Z.H.Li, Y.J.Li, J.Su, B.Guo, E.T.Li, K.J.Dong, X.X.Bai, Z.C.Li, J.C.Liu, S.Q.Yan, Y.B.Wang, S.Zeng, G.Lian, B.X.Wang, S.J.Jin, X.Liu, W.J.Zhang, W.Z.Huang, Q.W.Fan, L.Gan, Z.D.Wu, W.P.Liu New determination of the proton spectroscopic factor in 9Be from the 13C(9Be, 8Li)14N angular distribution NUCLEAR REACTIONS 13C(9Be, 8Li)14N, 12,13C(9Be, 9Be), E=40 MeV; measured particle spectra, Eα, differential s(θ) using Q3D magnetic spectrometer at HI-13 tandem accelerator facility in Beijing. 9Be; deduced proton spectroscopic factor for g.s. Optical model and DWBA analysis. Comparison with previous experimental and theoretical studies. Relevance to astrophysical S factor for 8Li(p, γ)9Be reaction.
doi: 10.1103/PhysRevC.87.017601
2013SU07 Phys.Rev. C 87, 024312 (2013) J.Su, W.P.Liu, N.C.Shu, S.Q.Yan, Z.H.Li, B.Guo, W.Z.Huang, S.Zeng, E.T.Li, S.J.Jin, X.Liu, Y.B.Wang, G.Lian, Y.J.Li, Y.S.Chen, X.X.Bai, J.S.Wang, Y.Y.Yang, R.F.Chen, S.W.Xu, J.Hu, S.Z.Chen, S.B.Ma, J.L.Han, P.Ma, Q.Hu, J.B.Ma, X.G.Cao, S.L.Jin, Z.Bai, K.Yang, F.D.Shi, W.Zhang, Z.Chen, L.X.Liu, Q.Y.Lin, X.S.Yan, X.H.Zhang, F.Fu, J.J.He, X.Q.Li, C.He, M.S.Smith Reexamining the β decay of 53, 54Ni, 52, 53Co, 51Fe, and 50Mn RADIOACTIVITY 50Mn, 50Cr, 51Fe, 52,53Co, 53,54Ni(β+), (EC), (β+p)[from (58Ni, X), E=68.6 MeV/nucleon]; measured β-delayed protons, (proton)γ-coin, Eγ, Iγ, T1/2 at HIRFL facility in Lanzhou. Implications for r process. Comparison with previous experimental studies.
doi: 10.1103/PhysRevC.87.024312
2012GU18 Astrophys.J. 756, 193 (2012) B.Guo, Z.H.Li, M.Lugaro, J.Buntain, D.Y.Pang, Y.J.Li, J.Su, S.Q.Yan, X.X.Bai, Y.S.Chen, Q.W.Fan, S.J.Jin, A.I.Karakas, E.T.Li, Z.C.Li, G.Lian, J.C.Liu, X.Liu, J.R.Shi, N.C.Shu, B.X.Wang, Y.B.Wang, S.Zeng, W.P.Liu New Determination of the 13C(α, n)16O Reaction Rate and its Influence on the s-process Nucleosynthesis in AGB Stars NUCLEAR REACTIONS 12,13C(11B, 7Li), E=50 MeV; measured reaction products; deduced σ(θ), S-factors, stellar rates. Comparison with available data.
doi: 10.1088/0004-637X/756/2/193
2012LI14 Eur.Phys.J. A 48, 13 (2012); Erratum Eur.Phys.J. A 49, 106 (2013) Y.J.Li, Z.H.Li, E.T.Li, X.X.Bai, J.Su, B.Guo, B.X.Wang, S.Q.Yan, S.Zeng, Z.C.Li, J.C.Liu, X.Liu, S.J.Jin, Y.B.Wang, L.Y.Zhang, X.Q.Yu, L.Li, G.Lian, Q.W.Fan, W.P.Liu New determination of the astrophysical 13C(p, γ)14N S(E) factors and reaction rates via the 13C(7Li, 6He)14N reaction NUCLEAR REACTIONS 13C(7Li, 6He), (7Li, 7Li), E=34 MeV; measured reaction products using Q3D magnetic spectrometer; deduced astrophysical S-factor, σ(θ), spectroscopic factors, potential parameters, resonance parameters; calculated spectroscopic factors, reaction rates using DWBA code PTOLEMY. Comparison with other data.
doi: 10.1140/epja/i2012-12013-x
2012LI35 Chin.Phys.C 36, 716 (2012) X.Liu, Y.-B.Wang, Z.-H.Li, S.-J.Jin, B.-X.Wang, Y.-J.Li, E.-T.Li, X.-X.Bai, B.Guo, J.Su, S.Zeng, S.-Q.Yan, G.Lian, W.-Z.Huang, W.-P.Liu Angular distribution of 6He+p elastic scattering NUCLEAR REACTIONS 1H(6He, p), E(cm)=4.3 MeV; measured reaction products, Ep, Ip. 6He; deduced σ(θ), optical potential parameters. DWBA calculations, comparison with available data.
doi: 10.1088/1674-1137/36/8/006
2011LI18 Chin.Phys.Lett. 28, 052102 (2011) E.-T.Li, Z.-H.Li, J.Su, B.Guo, Y.-J.Li, S.-Q.Yan, X.-X.Bai, Y.-B.Wang, B.-X.Wang, G.Lian, S.Zeng, X.Fang, W.-J.Zhao, W.-P.Liu Astrophysical Rates for the 6He(p, γ)7Li Reaction NUCLEAR REACTIONS 1H(6He, γ), 2H(6He, n), E(cm)=9.1 MeV; measured reaction products; deduced σ(θ), S-factors, temperature-dependent reaction rates. Comparison with DWBA analysis, REACLIB library.
doi: 10.1088/0256-307X/
2011LI55 J.Phys.:Conf.Ser. 312, 042013 (2011) W.P.Liu, Z.H.Li, B.Guo, Y.B.Wang, J.Su, X.X.Bai, G.Lian, B.X.Wang, S.Q.Yan, S.Zeng, Y.J.Li, E.T.Li, S.J.Jin, X.Liu Current progress of nuclear astrophysical reaction and decay study at CIAE NUCLEAR REACTIONS 2H(12N, 13O), E(cm)=8.4 MeV; measured reaction products using telescope with ΔE silicon and double-sided silicon strip detector and PPAC; deduced σ(θ); calculated σ(θ) using optical potential plus CN contribution. 7Li(6Li, 7Li), E(cm)=0.02-0.07 MeV; measured reaction products; deduced 6Li(n, γ) σ using spectroscopic factor. RADIOACTIVITY 147Sm(α)[in metal Sm and Sm2O3]; measured Eα, Iα; deduced T1/2.
doi: 10.1088/1742-6596/312/4/042013
2010JI02 Chin.Phys.Lett. 27, 032102 (2010) S.-J.Jin, Y.-B.Wang, B.-X.Wang, X.-X.Bai, X.Fang, B.Guo, E.-T.Li, Y.-J.Li, Z.-H.Li, G.Lian, J.Su, s.-Q.Yan, S.Zeng, Z.-E.Yao, W.-P.Liu Excited States in 18Ne Studied via 17F+p NUCLEAR REACTIONS 1H(17F, α), (17F, γ), E=55.5 MeV; measured recoil nuclei, Eα, Iα; deduced σ(θ), excitation function, 18Ne resonance states, J, π.
doi: 10.1088/0256-307X/27/3/032102
2010LI19 Eur.Phys.J. A 44, 1 (2010) Z.H.Li, E.T.Li, B.Guo, X.X.Bai, Y.J.Li, S.Q.Yan, Y.B.Wang, G.Lian, J.Su, B.X.Wang, S.Zeng, X.Fang, W.P.Liu First measurement of the 2H(6He, 7Li)n angular distribution and proton spectroscopic factor in 7Li NUCLEAR REACTIONS 2H(7Li, 6He)n, E=46 MeV; measured reaction products; deduced σ(θ), proton spectroscopic factor of 7Li ground state, optical potential parameters. Comparison with DWBA calculations.
doi: 10.1140/epja/i2010-10944-8
2010LI37 Nucl.Phys. A834, 651c (2010) W.P.Liu, Z.H.Li, X.X.Bai, Y.B.Wang, G.Lian, B.Guo, J.Su, S.Zeng, B.X.Wang, S.Q.Yan, Y.J.Li, E.T.Li Lithium induced nuclear reactions of astrophysical interest NUCLEAR REACTIONS 7Li(6Li, 7Li), E=tandem; measured E(particle), I(particle, θ); deduced spectroscopic factor, σ. 6Li(n, γ), E=0.01-0.1 MeV; deduced σ. Comparison with other data and systems, calculations.
doi: 10.1016/j.nuclphysa.2010.01.114
2010LI38 Nucl.Phys. A834, 661c (2010) Z.H.Li, J.Su, B.Guo, E.T.Li, Z.C.Li, X.X.Bai, Y.J.Li, J.C.Liu, S.Q.Yan, B.X.Wang, Y.B.Wang, G.Lian, S.Zeng, X.Fang, W.P.Liu, Y.S.Chen, N.C.Shu, Q.W.Fan 2H(6He, 7Li)n, 12C(7Li, 6He)13N reactions and 12C(p, γ)13N astrophysical S(E) factors NUCLEAR REACTIONS 2H(6He, 7Li), E not given; 12C(7Li, 6He), E=44.0 MeV; measured σ(θ); deduced 12C(p, γ) S-factor; calculated S-factor using DWBA and asymptotic normalization coefficient. Comparison with other data.
doi: 10.1016/j.nuclphysa.2010.01.117
2010SU08 Chin.Phys.Lett. 27, 052101 (2010) J.Su, Z.-H.Li, B.Guo, X.-X.Bai, Z.-C.Li, J.-C.Liu, Y.-B.Wang, G.Lian, S.Zeng, B.-X.Wang, S.-Q.Yan, Y.-J.Li, E.-T.Li, Q.-W.Fan, W.-P.Liu Neutron Spectroscopic Factors of 7Li and Astrophysical 6Li(n, γ)7Li Reaction Rates NUCLEAR REACTIONS 7Li(6Li, 7Li), (6Li, 6Li), E=23.7 MeV; measured reaction products; deduced σ(θ), spectroscopic factors. NUCLEAR REACTIONS 6Li(p, γ), (n, γ), E(cm)<1.2 MeV; calculated astrophysical reaction rates, S-factors. DWBA analysis.
doi: 10.1088/0256-307X/27/5/052101
2010SU30 Eur.Phys.J. A 46, 69 (2010) J.Su, Z.H.Li, L.C.Zhu, G.Lian, X.X.Bai, Y.B.Wang, B.Guo, B.X.Wang, S.Q.Yan, S.Zeng, Y.J.Li, E.T.Li, S.J.Jin, X.Liu, Q.W.Fan, J.L.Zhang, X.Y.Jiang, J.X.Lu, X.F.Lan, X.Z.Tang, W.P.Liu Alpha decay half-life of 147Sm in metal samarium and Sm2O3 RADIOACTIVITY 147Sm(α); measured Eα, Iα for metalic Sm and Sm oxide; deduced T1/2. Halflives in both forms are different.
doi: 10.1140/epja/i2010-11028-7
2010WA18 Nucl.Phys. A834, 100c (2010) Y.B.Wang, B.X.Wang, S.J.Jin, X.Qin, X.X.Bai, W.P.Liu, Z.H.Li, G.Lian, S.Zeng, B.Guo, S.Q.Yan, J.Su, Y.J.Li, E.T.Li, X.Fang Elastic resonance scattering of 13N+p and 17F+p NUCLEAR REACTIONS 2H(12C, 13N), (16O, 17F), E not given; 1H(13N, 13N), (17F, 17F), E=47.8 MeV; measured reaction products, proton spectrum; 14O, 18Ne; deduced resonance parameters, J, π, σ(θ); R-matrix analysis.
doi: 10.1016/j.nuclphysa.2010.01.030
2009LI27 Chin.Phys.Lett. 26, 072401 (2009) E.-T.Li, Z.-H.Li, Y.-J.Li, S.-Q.Yan, X.-X.Bai, B.Guo, J.Su, Y.-B.Wang, B.-X.Wang, G.Lian, S.Zeng, X.Fang, W.-J.Zhao, W.-P.Liu Angular Distribution of the 12C(6He, 7Li)11B Reaction NUCLEAR REACTIONS 12C(6He, 7Li), E = 34.6 MeV; measured σ(θ). comparison with DWBA calculation.
doi: 10.1088/0256-307X/26/7/072401
2009WA25 Chin.Phys.C 33, 181 (2009) Y.-B.Wang, X.Qin, B.-X.Wang, W.-P.Liu, Z.-H.Li, X.-X.Bai, G.Lian, B.Guo, S.Zeng, J.Su, Y.-J.Li, C.Jiang Simulation and analysis of 13N+p elastic resonance scattering NUCLEAR REACTIONS 1H(13N, p), E=47.8 MeV; measured reaction products; 14O; deduced σ, resonance parameters, J, π. Monte-Carlo simulations.
doi: 10.1088/1674-1137/33/3/004
2009WA29 Chin.Phys.C 33, Supplement 1, 79 (2009) M.Wang, Y.-S.Chen, Z.-H.Li, W.-P.Liu, N.-C.Shu Calculation of astrophysical reaction rate of 82Ge(n, γ)83Ge NUCLEAR REACTIONS 82Ge(n, γ), E<1 MeV; 82Ge(d, p), E(cm)=7.9 MeV; analyzed σ(θ); calculated σ(θ), σ; deduced astrophysical reaction rate. DWBA analysis.
doi: 10.1088/1674-1137/33/S1/026
2008LI02 Chin.Phys.Lett. 25, 70 (2008) G.Lian, J.Su, B-X.Wang, C.Jiang, X.-X.Bai, S.Zeng, Y.-N.Zheng, S.-Y.Zhu, L.-H.Zhu, W.-P.Liu, Z.-H.Li, Y.-B.Wang, B.Guo, Y.-J.Li, X.Qin Enhancement of β+-Decay Rate of 22Na in Metal Pd at Low Temperature RADIOACTIVITY 22Na(β+); measured Eγ, Iγ. Deduced evidence for temperature dependence of half life for decays in metallic environment.
doi: 10.1088/0256-307X/25/1/020
2008LI03 Chin.Phys.Lett. 25, 455 (2008) Y.-J.Li, Z.-H.Li, B.Guo, Y.-B.Wang, X.-X.Bai, J.Su, G.Lian, S.Zeng, B.-X.Wang, X.Qin, C.Jiang, W.-P.Liu, W.-J.Zhao Measurement of Angular Distribution for the 8Li(p, d)7Li Reaction NUCLEAR REACTIONS 1H(8Li, 7Li), E=39.8 MeV; measured particle energies and yields. 8Li(p, d), E(cm)=4.0 MeV; deduced cross sections and backward anglular distributions.
doi: 10.1088/0256-307X/25/2/028
2008WA09 Phys.Rev. C 77, 044304 (2008) Y.B.Wang, B.X.Wang, X.Qin, X.X.Bai, B.Guo, C.Jiang, Y.J.Li, Z.H.Li, G.Lian, J.Su, S.Zeng, W.P.Liu 13N + p elastic resonance scattering via a thick-target method NUCLEAR REACTIONS 2H(12C, 13N), E=72 MeV; measured excitation function. 1H(13N, 13N), E=47.8 MeV; measured proton energy, σ(θ). 13N, 14O; deduced levels, J, π, resonance parameters.
doi: 10.1103/PhysRevC.77.044304
2007GU01 J.Phys.(London) G34, 103 (2007) B.Guo, Z.H.Li, W.P.Liu, X.X.Bai Determination of astrophysical 11C(p, γ)12N reaction rate from the asymptotic normalization coefficients of 12B → 11B + n NUCLEAR REACTIONS 11B(d, p), E ≈ 12 MeV; analyzed σ(E, θ). 12B deduced asymptotic normalization coefficient for virtual neutron decay. 11C(p, γ), E(cm) ≈ 0.1-0.7 MeV; calculated astrophysical S-factor. 12N deduced excited states widths.
doi: 10.1088/0954-3899/34/1/006
2007GU18 Chin.Phys.Lett. 24, 2544 (2007) B.Guo, Z-H.Li, W.-P.Liu, X.-X.Bai Test of Determination of (p, γ) Astrophysical S-Factors Using the Asymptotic Normalization Coefficients from Neutron Transfer Reactions NUCLEAR REACTIONS 16O(d, p), E not given; analyzed angular distributions to extract ANCs using DWBA and adiabatic wave approximation. 16O(p, γ), E < 1.5 MeV; deduced astrophysical S-factors.
doi: 10.1088/0256-307X/24/9/022
2007TE09 Phys.Lett. B 650, 129 (2007) T.Teranishi, S.Kubono, H.Yamaguchi, J.J.He, A.Saito, H.Fujikawa, G.Amadio, M.Niikura, S.Shimoura, Y.Wakabayashi, S.Nishimura, M.Nishimura, J.Y.Moon, C.S.Lee, A.Odahara, D.Sohler, L.H.Khiem, Z.H.Li, G.Lian, W.P.Liu Single-particle resonance levels in 14O examined by 13N + p elastic resonance scattering NUCLEAR REACTIONS 1H(13N, 13N), E(cm)=0.4-3.3 MeV; measured elastic scattering σ(θ) and fitted with R-matrix calculation. 14O deduced levels, widths, J, π, spectroscopic factor.
doi: 10.1016/j.physletb.2007.05.013
2006GU01 Chin.Phys.Lett. 23, 52 (2006) B.Guo, Z.-H.Li, W.-P.Liu, X.-X.Bai Asymptotic Normalization Coefficient of 27P → 26Si + p and Radius of 27P Halo NUCLEAR REACTIONS 26Mg(d, p), E=12 MeV; analyzed σ(θ). 27P deduced asymptotic normalization coefficient for virtual proton decay, proton halo radius.
doi: 10.1088/0256-307X/23/1/016
2006GU09 Phys.Rev. C 73, 048801 (2006) B.Guo, Z.H.Li, X.X.Bai, W.P.Liu, N.C.Shu, Y.S.Chen Determination of the astrophysical 26Si(p, γ)27P reaction rate from the asymptotic normalization coefficients of 27Mg → 26Mg + n NUCLEAR REACTIONS 26Mg(d, p), E=12 MeV; analyzed σ(E, θ); deduced asymptotic normalization coefficients. 26Si(p, γ), E=low; deduced astrophysical reaction rate.
doi: 10.1103/PhysRevC.73.048801
2006GU36 High Energy Phys. and Nucl.Phys. (China), Supplement 2, 30, 183 (2006) B.Guo, Z.-H.Li, W.-P.Liu, X.-X.Bai Study of Halo for the Ground State and Proton Widths for the First Two Excited States of 27P
2006LI48 Phys.Rev. C 74, 035801 (2006) Z.H.Li, B.Guo, S.Q.Yan, G.Lian, X.X.Bai, Y.B.Wang, S.Zeng, J.Su, B.X.Wang, W.P.Liu, N.C.Shu, Y.S.Chen, H.W.Chang, L.Y.Jiang 13N(d, n)14O reaction and the astrophysical 13N(p, γ)14O reaction rate NUCLEAR REACTIONS 2H(13N, n), E(cm)=8.9 MeV; measured σ(θ); deduced asymptotic normalization coefficient. 13N(p, γ), E(cm)=0-1.0 MeV; deduced astrophysical S-factors, reaction rate.
doi: 10.1103/PhysRevC.74.035801
2006LI62 Int.J.Mod.Phys. E15, 1899 (2006) W.-P.Liu, Z.-H.Li, X.-X.Bai, Y.-B.Wang, G.Lian, B.Guo, S.Zeng, S.-Q.Yan, B.-X.Wang, J.Su, N.-C.Shu, Y.-S.Chen Indirect measurements of nuclear astrophysics reactions using unstable nuclear beams NUCLEAR REACTIONS 2H(7Be, n), (11C, n), (8Li, p), (13N, n), E(cm) ≈ 6-9 MeV; analyzed σ, asymptotic normalization coefficients. 7Be, 11C, 8Li, 13N(p, γ), E=low; deduced astrophysical S-factors, reaction rates.
doi: 10.1142/S0218301306005514
2006SU01 Chin.Phys.Lett. 23, 55 (2006) J.Su, Z.-H.Li, B.Guo, W.-P.Liu, X.-X.Bai, S.Zeng, G.Lian, S.-Q.Yan, B.-X.Wang, Y.-B.Wang Astrophysical Reaction Rates of the 8Li(p, g)9Beg.s Direct Capture Reaction NUCLEAR REACTIONS 2H(8Li, n), E=40 MeV; measured σ(θ); deduced optical potential parameters. 8Li(p, γ), E(cm) ≈ 0-2 MeV; deduced astrophysical S-factors, reaction rates.
doi: 10.1088/0256-307X/23/1/017
2006TR08 Can.J.Phys. 84, 325 (2006) M.Trinczek, S.Lapi, B.Guo, F.Ames, K.R.Buckley, J.M.D'Auria, K.Jayamanna, W.P.Liu, C.Ruiz, T.J.Ruth Production of intense radioactive beams at ISAC using low-energy protons NUCLEAR REACTIONS 14N(p, α), (p, n), E=13 MeV; measured yields. Application to radioactive beam production discussed.
doi: 10.1139/P06-058
2005GU29 Nucl.Phys. A761, 162 (2005) B.Guo, Z.H.Li, W.P.Liu, X.X.Bai, G.Lian, S.Q.Yan, B.X.Wang, S.Zeng, J.Su, Y.Lu The 8Li(d, p)9Li reaction and astrophysical 8B(p, γ)9C reaction rate NUCLEAR REACTIONS 2H(8Li, 9Li), E(cm)=7.8 MeV; measured σ(θ); deduced asymptotic normalization coefficient. 8B(p, γ), E=low; calculated astrophysical S-factor. DWBA analysis, inverse kinematics, comparison with data.
doi: 10.1016/j.nuclphysa.2005.07.013
2005LI19 Phys.Rev. C 71, 052801 (2005) Z.H.Li, W.P.Liu, X.X.Bai, B.Guo, G.Lian, S.Q.Yan, B.X.Wang, S.Zeng, Y.Lu, J.Su, Y.S.Chen, K.S.Wu, N.C.Shu, T.Kajino The 8Li(d, p)9Li reaction and the astrophysical 8Li(n, γ)9Li reaction rate NUCLEAR REACTIONS 2H(8Li, 9Li), E=39 MeV; measured particle spectra, σ(θ). 8Li(n, γ), E=low; deduced astrophysical reaction rates.
doi: 10.1103/PhysRevC.71.052801
2005LI35 Chin.Phys.Lett. 22, 1870 (2005) Z.H.Li, B.Guo, W.-P.Liu, X.-X.Bai, G.Lian, J.Su, S.-Q.Yan, B.-X.Wang, S.Zeng Radius of 9C from the Asymptotic Normalization Coefficient NUCLEAR REACTIONS 2H(8Li, p), E(cm)=7.8 MeV; measured σ(θ); deduced asymptotic normalization coefficients. 9C deduced radius, density distributions, halo structure.
doi: 10.1088/0256-307X/22/8/013
2005SH39 Nucl.Phys. A758, 419c (2005) N.-C.Shu, Y.-S.Chen, K.-S.Wu, X.-X.Bai, Z.-H.Li, W.-P.Liu The 11C(p, γ)12N reaction rate and the conversion of 3He into CNO NUCLEAR REACTIONS 11C(p, γ), E=low; analyzed S-factors, related data; deduced astrophysical reaction rates.
doi: 10.1016/j.nuclphysa.2005.05.077
2005ZE03 Chin.Phys.Lett. 22, 2219 (2005) S.Zeng, W.-P.Liu, Z.-H.Li, X.-X.Bai, S.-Q.Yan, B.-X.Wang, G.Lian, J.Su Measurement of 2H(8Li, 9Be)n Reaction Relevant to Primordial Nucleosynthesis NUCLEAR REACTIONS 2H(8Li, 9Be), E=40.38 MeV; measured particle spectra, σ(θ); deduced astrophysical S-factors.
doi: 10.1088/0256-307X/22/9/022
2002LI17 Chin.Phys.Lett. 19, 306 (2002) Z.-H.Li, W.-P.Liu, X.-X.Bai, Y.-B.Wang, G.Lian, Z.-C.Li, Q.-B.Shen, C.-J.Lin, S.Zeng, C.-B.Fu Search for the Halo Effect in the 1H(6He, 6Li)n Reaction NUCLEAR REACTIONS 1H(6He, 6Li), E=4.17 MeV/nucleon; measured σ(E, θ). 6He, 6Li deduced halo structure. DWBA analysis.
doi: 10.1088/0256-307X/19/3/306
2001LI56 Chin.Phys.Lett. 18, 1449 (2001) W.-P.Liu, M.Hellstrom, R.Collatz, J.Benlliure, L.Chulkov, D.Cortina Gil, F.Farget, H.Grawe, Z.Hu, N.Iwasa, M.Pfutzner, A.Piechaczek, R.Raabe, I.Reusen, E.Roeckl, G.Vancraeynest, A.Wohr Precise Determination of 40Ti Mass by Measuring the 40Sc Isospin Analogue State RADIOACTIVITY 40Ti(EC) [from 9Be(58Ni, X)]; measured β-delayed proton spectra. 40Sc deduced IAS energy. 40Ti deduced mass.
doi: 10.1088/0256-307X/18/11/307
1999WA25 Chin.Phys.Lett. 16, 873 (1999) Y.-B.Wang, W.-P.Liu, X.-X.Bai, Z.-C.Li, A.-L.Li, S.-H.Zhou, X.-F.Zhu, X.-M.Li, G.-K.He, G.Guo, G.Lian, X.-D.Tang Angular Distribution for 7Be(d, n)8B Reaction at Ec.m. = 8.3 MeV and the Astrophysical S17(0) Factor for 7Be(p, γ)8B Reaction NUCLEAR REACTIONS 2H(7Be, n), E(cm)=8.3 MeV; measured σ(θ), σ. 7Be(p, γ), E=low; deduced reaction S-factor. Radioactive beam, DWBA calculations. Nuclear astrophysics.
doi: 10.1088/0256-307X/16/12/006
1995LU22 Chin.J.Nucl.Phys. 17, No 2, 185 (1995) J.Lu, S.-L.Li, H.-S.Xu, Y.-T.Zhu, W.-P.Liu, X.-X.Bai A High Resolution Ionization Chamber Detector RADIOACTIVITY 241Am(α); measured ionization chamber detector energy resolution vs gas pressure. High resolution.
1994LI63 Chin.J.Nucl.Phys. 16, No 3, 255 (1994) A.-L.Li, X.-X.Bai, X.-Z.Wang, Y.-F.Wang, J.-C.Meng, W.-P.Liu, Y.Yuan, T.-H.Chih, S.-N.Huang Experimental Study of the Prompt Neutron Spectra of 238U Fission Induced by Fast Neutrons NUCLEAR REACTIONS 238U(n, F), E=10.17, 12.12 MeV; measured prompt fission neutron spectra, fission (fragment)n-coin; deduced Maxwellian temperatures. Double tof, multi-segment fission chamber, two ST-451 liquid scintillator neutron detectors.
1990LI05 Nucl.Instrum.Methods Phys.Res. A287, 476 (1990) W.P.Liu, T.Kubo, H.Kumagai, T.Nakagawa, T.Suzuki, M.Yanokura, I.Tanihata, T.Ito, T.Kashiwagi, J.Kikuchi, H.Yamaguchi, T.Doke, H.Murakami, T.Yanagimachi, N.Hasebe Identification of Projectile Fragments Using Position Sensitive Silicon Detectors NUCLEAR REACTIONS 9Be(40Ca, X), E=16 MeV/nucleon; measured fragment total energy, tof, energy loss; deduced fragment charge state, mass, Z. Position sensitive Si detector.
doi: 10.1016/0168-9002(90)91566-T
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