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NSR database version of April 24, 2024.

Search: Author = E.T.Li

Found 35 matches.

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2023ZH17      Phys.Rev. C 107, 045809 (2023)

S.Zhang, G.Li, W.Jiang, D.X.Wang, J.Ren, M.Huang, E.T.Li, J.Y.Tang, X.C.Ruan, H.W.Wang, Z.H.Li, Y.S.Chen, L.X.Liu, X.X.Li, Q.W.Fan, R.R.Fan, X.R.Hu, J.C.Wang, X.Li, D.D.Niu, N.Song, M.Gu

Measurement of the 159Tb (n, γ) cross section at the CSNS Back-n facility

NUCLEAR REACTIONS 159Tb(n, γ), E=0.002-1 MeV; measured neutron Time-of-Flight, Eγ, Iγ; deduced σ(E), resonance parameters, Maxwellian-averaged σ (kT=5-100 keV), astrophysical reaction rate. R-matrix analysis (SAMMY code) to obtain resonance parameters and compare to JEFF-3.3 evaluations, recommended data from Mughabghab and ENDF/B-VIII.0. Comparison of cross-section data to other experimental results, TALYS-1.9 calculations, data from KADoNiS-v0.3, KADoNiS-v1.0, JEFF-3.3, ENDF/B-VIII.0. Analyzed impact of the obtained data on the time evolution of nuclear abundances of 159Tb, 160Tb, 160Dy, 161Dy, 162Dy, 163Dy, 164Dy, 163Ho, 165Ho, 164Er, 166Er, 167Er. Four C6D6 detectors. Neutron beam from Back-n Facility of the China spallation neutron source (CSNS).

doi: 10.1103/PhysRevC.107.045809
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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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Data from this article have been entered in the XUNDL database. For more information, click here.


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


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


2021GA21      Chin.Phys.C 45, 054105 (2021)

L.Gan, Z.-H.Li, H.-B.Sun, S.-P.Hu, E.-T.Li, J.Zhong

Systematic study of the Woods-Saxon potential parameters between heavy-ions

NUCLEAR REACTIONS 90Zr(12C, 12C), E=66 MeV; 58Ni(11B, 11B), 12,13C, 16O, 19F, 40Ca, 64Ni, 90Zr, 116Sn, 169Tm, 208Pb, 209Bi(12C, 12C), 64,68Zn, 209Bi(16O, 16O), E=25-420 MeV; analyzed available data; deduced Woods-Saxon potential parameters using experimental elastic scattering σ(θ).

doi: 10.1088/1674-1137/abe84f
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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
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0225.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0087.


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.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0187.


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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2018ZH06      Phys.Rev. C 97, 014611 (2018)

G.L.Zhang, G.X.Zhang, S.P.Hu, Y.J.Yao, J.B.Xiang, H.Q.Zhang, J.Lubian, J.L.Ferreira, B.Paes, E.N.Cardozo, H.B.Sun, J.J.Valiente-Dobon, D.Testov, A.Goasduff, P.R.John, M.Siciliano, F.Galtarossa, R.Francesco, D.Mengoni, D.Bazzacco, E.T.Li, X.Hao, W.W.Qu

One-neutron stripping processes to excited states of 90Y* in the 89Y(6Li, 5Li)90Y* reaction

NUCLEAR REACTIONS 89Y(6Li, 5Li)90Y*, E=22, 34 MeV; measured in-beam and off-beam Eγ, Iγ, γγ- and pγ-coin, ΔE-E for protons, deuterons, tritons, and α particles, one-neutron stripping σ(E) using GALILEO array for γ rays and 4π Si-ball EUCLIDES for particles at the Tandem-XTU accelerator of Legnaro National Laboratory. 90Y, 93Mo; deduced level schemes. Comparisons of cross sections with parameter-free coupled reaction channel calculations.

doi: 10.1103/PhysRevC.97.014611
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2438.


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


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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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.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2064. Data from this article have been entered in the XUNDL database. For more information, click here.


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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0075. Data from this article have been entered in the XUNDL database. For more information, click here.


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


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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2011HE09      Eur.Phys.J. A 47, 67 (2011)

J.J.He, J.Hu, S.W.Xu, Z.Q.Chen, X.Y.Zhang, J.S.Wang, H.W.Wang, W.D.Tian, X.Q.Yu, L.Y.Zhang, L.Li, Y.Y.Yang, P.Ma, X.H.Zhang, J.Su, E.T.Li, Z.G.Hu, Z.Y.Guo, X.Xu, X.H.Yuan, W.Lu, Y.H.Yu, Y.D.Zang, S.W.Ye, R.P.Ye, J.D.Chen, S.L.Jin, C.M.Du, S.T.Wang, J.B.Ma, L.X.Liu, Z.Bai, X.Q.Li, X.G.Lei, Z.Y.Sun, Y.H.Zhang, X.H.Zhou, H.S.Xu

Study of proton resonances in 18Ne via resonant elastic scattering of 17F + p and its astrophysical implication in the stellar reaction of 14O(α, p)17F

NUCLEAR REACTIONS 1H, 12C(17F, X), E=4.22 MeV/nucleon; measured E(particle), I(particle, θ); deduced σ(θ), R-matrix resonance parameters; calculated σ(θ), α spectroscopic factors, resonant reaction rates using multichannel R-matrix.

doi: 10.1140/epja/i2011-11067-6
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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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