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NSR database version of April 27, 2024.

Search: Author = N.C.Shu

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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, ^{233,234,235,238}U, 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, 54}Ni, ^{52, 53}Co, 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, T_1/2 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, T_1/2. 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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