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NSR database version of April 11, 2024.

Search: Author = X.C.Du

Found 8 matches.

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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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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.


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.


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


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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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.


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.


2009FE09      Chin.Phys.C 33, Supplement 1, 52 (2009)

S.-Q.Feng, X.-C.Du

Dependence of multiplicity and transverse energy distributions on nuclear geometry at RHIC

doi: 10.1088/1674-1137/33/S1/017
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