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NSR database version of April 27, 2024.

Search: Author = K.S.Wu

Found 4 matches.

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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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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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2003WU01      Chin.Phys.Lett. 20, 49 (2003)

K.-S.Wu, Y.-S.Chen, Z.-H.Liu, C.-J.Lin, H.-Q.Zhang

Calculation of Cross Section of Radiative Halo-Neutron Capture by ¹²C at Stellar Energy with the Asymptotic Normalization Coefficient Method

NUCLEAR REACTIONS ¹²C(n, γ), E=0-1 MeV; calculated σ. Asymptotic normalization coefficient method, comparison with data.

doi: 10.1088/0256-307X/20/1/315
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