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NSR database version of April 24, 2024.

Search: Author = D.Nan

Found 3 matches.

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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.


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.


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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