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NSR database version of April 11, 2024.

Search: Author = N.C.Shu

Found 23 matches.

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2024LI04      Phys.Rev. C 109, 014603 (2024)

L.-L.Liu, Y.-Y.Liu, X.-L.Huang, J.-M.Wang, Y.-J.Chen, N.-Ch.Shu, Zh.-G.Ge

Influence of the spin cut-off parameter on the isomeric cross-section ratio of the (n, 2n) reaction within the Huizenga-Vandenbosch method

doi: 10.1103/PhysRevC.109.014603
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2022LI65      Chin.Phys.C 46, 124101 (2022)

L.-L.Liu, X.-Z.Wu, Y.-J.Chen, C.-W.Shen, Z.-X.Li, Z.-G.Ge, N.-C.Shu

Influence of the neck parameter on the fission dynamics within the two-center shell model parametrization

NUCLEAR REACTIONS 235U(n, F), E=14 MeV; calculated the total kinetic energy (TKE) distributions.

doi: 10.1088/1674-1137/ac8867
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2022WA26      Phys.Rev. C 106, L021304 (2022)

Z.A.Wang, J.C.Pei, Y.J.Chen, C.Y.Qiao, F.R.Xu, Z.G.Ge, N.C.Shu

Bayesian approach to heterogeneous data fusion of imperfect fission yields for augmented evaluations

NUCLEAR REACTIONS 238U(n, F), E<20 MeV; analyzed experimental data; calculated cumulative fission yields of 99Mo, 135Xe, 140Ba, 147Nd fragments, independent fission yields. Bayesian neural networks (BNNs) algorithm for machine learning.

doi: 10.1103/PhysRevC.106.L021304
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2021QI04      Phys.Rev. C 103, 034621 (2021)

C.Y.Qiao, J.C.Pei, Z.A.Wang, Y.Qiang, Y.J.Chen, N.C.Shu, Z.G.Ge

Bayesian evaluation of charge yields of fission fragments of 239U

NUCLEAR REACTIONS 232,233Th, 239Pu(n, F), E=14 MeV; 239Pu, 244Cm(n, F), E=0.5 MeV; 255Fm(n, F), E=0.025 eV; analyzed one-layer and two-layer Bayesian neural network (BNN) learning results of charge yields taken from JENDL. 235U(n, F), E=0.025 eV and 0.5, 14 MeV; predicted BNN fission charge yields. 238U(n, F)239U*, E=0.5 MeV; calculated and evaluated BNN fission charge yields. Double-layered Bayesian neural network (BNN) to learn and predict charge yields of fission fragments; deduced better performance of double-layer network better than that of the single-layer network with same number of neurons. Comparison with experimental data.

doi: 10.1103/PhysRevC.103.034621
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2016CA03      Nucl.Data Sheets 131, 1 (2016)

R.Capote, Y.-J.Chen, F.-J.Hambsch, N.V.Kornilov, J.P.Lestone, O.Litaize, B.Morillon, D.Neudecker, S.Oberstedt, T.Ohsawa, N.Otuka, V.G.Pronyaev, A.Saxena, O.Serot, O.A.Shcherbakov, N.-C.Shu, D.L.Smith, P.Talou, A.Trkov, A.C.Tudora, R.Vogt, A.S.Vorobyev

Prompt Fission Neutron Spectra of Actinides

NUCLEAR REACTIONS 232Th, 233,234,235,238U, 237Np, 239Pu(n, F), E<30 MeV; calculated prompt fission En, In; Comparison with available data.

doi: 10.1016/j.nds.2015.12.002
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset33084.

2015SH17      Chin.Phys.C 39, 054101 (2015)

N.-C.Shu, M.Jia, Y.-J.Chen, T.J.Liu

Prompt fission neutron spectra of n+235U above the (n, nf) fission threshold

NUCLEAR REACTIONS 235U(n, F), E=7, 14.7 MeV; calculated prompt fission neutron spectra, multiple-chance fission contributions.

doi: 10.1088/1674-1137/39/5/054101
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2014CH17      Chin.Phys.C 38, 054001 (2014)

Y.-J.Chen, M.Jia, T.-J.Liu, N.-C.Shu

Calculation of prompt fission neutron spectrum for 233U(n, f) reaction by the semi-empirical method

NUCLEAR REACTIONS 233U(n, F), E<6 MeV; calculated σ(E), prompt neutron spectra, energy partition between fragments. Comparison with available data.

doi: 10.1088/1674-1137/38/5/054001
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2405. 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.

2012CH20      Chin.Phys.C 36, 322 (2012)

Y.-J.Chen, M.Jia, X.Tao, J.Qian, T.-J.Liu, N.-C.Shu

Calculation of prompt fission neutron spectra for 235U(n, f)

NUCLEAR REACTIONS 235U(n, F), E<5 MeV; calculated prompt fission neutron spectrum. Comparison with available data.

doi: 10.1088/1674-1137/36/4/005
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2012CH33      Int.J.Mod.Phys. E21, 1250073 (2012)

Y.-J.Chen, J.Qian, T.-J.Liu, Z.-X.Li, X.-Z.Wu, N.-C.Shu

Energy partition in 235U fission reaction induced by thermal neutron

NUCLEAR REACTIONS 235U(n, F), E=thermal; 235U(n, F), E=5.55 MeV; analyzed available data; deduced partition of the total excitation energy between fission fragments. Comparison with available data.

doi: 10.1142/S0218301312500735
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0072.

2011SH36      J.Korean Phys.Soc. 59, 1353s (2011)

N.-C.Shu, Y.-J.Chen, T.-J.Liu, Z.-J.Sun, X.-Z.Wu, J.Qian, R.-R.Xu, T.-S.Fan

Semi-Empirical Study on the Yield Energy-Dependence of the 235U + n Fission

COMPILATION 235U(n, F), E-0-30 MeV; compiled, evaluated 87Kr, 144Ce, 161Tb yields vs neutron energy; deduced parameters using model based on Brosa's idea. 235U(n, F), E=thermal, 0.5-18 MeV, 20 MeV; calculated mass yields using TALYS code and Brosa-like model. Comparison with available data.

doi: 10.3938/jkps.59.1353
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2010HO09      Chin.Phys.Lett. 27, 082601 (2010)

S.-Q.Hou, K.-S.Wu, Y.-S.Chen, N.-C.Shu, Z.-H.Li

The Main Path to C, N, O Elements in Big Bang Nucleosynthesis

NUCLEAR REACTIONS 8Li(d, p), E(cm)=7.8 MeV; 8Li(n, γ), 9Li(α, n), E not given; calculated yields; deduced production of C, N, O elements in standard Big Bang nucleosynthesis.

RADIOACTIVITY 12B(β-); calculated yields of 12C.

doi: 10.1088/0256-307X/27/8/082601
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0062.

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
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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
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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0483.

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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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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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0047.

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
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2005XU04      Phys.Rev. C 71, 054318 (2005)

S.-W.Xu, Z.-K.Li, Y.-X.Xie, Q.-Y.Pan, W.-X.Huang, X.-D.Wang, Y.Yu, Y.-B.Xing, N.-C.Shu, Y.-S.Chen, F.-R.Xu, K.Wang

β-delayed proton decays near the proton drip line

RADIOACTIVITY 81Zr, 85Mo, 89Ru, 92Rh, 93Pd, 121Ce, 125Nd, 128Pm, 129Sm, 135,137Gd, 139Dy, 142Ho, 149Yb(β+p); measured β-delayed Eγ, Iγ, proton spectra, pγ-coin, T1/2. Comparison with model predictions.

NUCLEAR REACTIONS 92Mo, 106Cd(32S, 3n), E=151 MeV; 92Mo(36Ar, 3n), E=169 MeV; 96Ru(36Ar, 3n), (36Ar, 3np), E=165, 174 MeV; 106Cd(36Ar, 3n), (36Ar, nα), E=176 MeV; 106Cd(40Ca, 4n), E=202 MeV; 112Sn(40Ca, 3n), E=185 MeV; measured σ.

doi: 10.1103/PhysRevC.71.054318
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2003SH25      Chin.Phys.Lett. 20, 1470 (2003)

N.-C.Shu, D.W.Bardayan, J.C.Blackmon, Y.-S.Chen, R.L.Kozub, P.D.Parker, M.S.Smith

New Astrophysical Reaction Rates for 18F(p, α)15O and 18F(p, γ)19Ne

NUCLEAR REACTIONS 18F(p, α), (p, γ), E=low; analyzed data; calculated astrophysical reaction rates.

doi: 10.1088/0256-307X/20/9/317
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