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NSR database version of April 11, 2024.

Search: Author = S.Q.Yan

Found 47 matches.

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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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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
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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
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2022OR04      Phys.Rev. C 106, 064301 (2022)

R.Orlandi, H.Makii, K.Nishio, K.Hirose, M.Asai, K.Tsukada, T.K.Sato, Y.Ito, F.Suzaki, Y.Nagame, A.N.Andreyev, E.Ideguchi, N.Aoi, T.T.Pham, S.Q.Yan, Y.P.Shen, B.Gao, G.Li

New K isomers in 248Cf

NUCLEAR REACTIONS 249Cf(18O, 19O)248Cf, E=140.4 MeV; measured reaction products, Eγ, Iγ, γγ-coin, particleγ-coin. 248Cf; deduced levels, J, π, transitions from isomeric states, T1/2 for 2 low-ling transitions, B(E1). Discussed possible configuration of newly observed isomeric state at 950 keV to be two-quasineutron K=8- and the two-quasiproton K=5-. Comparison to other experimental data. Radioactive target. Si-detectors array combined with γ-ray detector array consisted of 4 Ge detectors and 4 4x5 inch LaBr3 scintillators at Tokai Tandem accelerator facility of the Japan Atomic Energy Agency (JAEA).

doi: 10.1103/PhysRevC.106.064301
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2021YA29      Astrophys.J. 919, 84 (2021)

S.Q.Yan, X.Y.Li, K.Nishio, M.Lugaro, Z.H.Li, H.Makii, M.Pignatari, Y.B.Wang, R.Orlandi, K.Hirose

The 59Fe(n, γ)60Fe Cross Section from the Surrogate Ratio Method and Its Effect on the 60Fe Nucleosynthesis

NUCLEAR REACTIONS 56,58Fe(18O, 16O), E=103 MeV; measured reaction products, Eγ, Iγ; deduced σ, Maxwellian-averaged σ. Comparison with TALYS calculations.

doi: 10.3847/1538-4357/ac12ce
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset32857.


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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0230. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0213. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset32770.


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
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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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0095. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0198. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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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
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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
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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
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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
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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
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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
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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
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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/
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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