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NSR database version of April 26, 2024.

Search: Author = L.H.Qiao

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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 Γ_p 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.

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.

2016YA09      Phys.Rev. C 94, 015804 (2016)

S.Q.Yan, Z.H.Li, Y.B.Wang, K.Nishio, H.Makii, J.Su, Y.J.Li, I.Nishinaka, K.Hirose, Y.L.Han, R.Orlandi, Y.P.Shen, B.Guo, S.Zeng, G.Lian, Y.S.Chen, X.X.Bai, L.H.Qiao, W.P.Liu

Examination of the surrogate ratio method for the determination of the ⁹³Zr (n, γ)⁹⁴Zr cross section with ^{90, 92}Zr(¹⁸O, ¹⁶O) ^{92, 94}Zr reactions

NUCLEAR REACTIONS ^90,92Zr(¹⁸O, ¹⁶O), E=117 MeV; measured Eγ, Iγ, (¹⁶O)γ-coin at the Tandem accelerator of JAEA facility. ^92,94Zr; measured γ-decay probability ratios. ⁹³Zr(n, γ), E>3 MeV; deduced σ(E) by surrogate ratio method, using reference cross sections of the ⁹¹Zr(n, γ)⁹²Zr reaction from ENDF/B-VII.1, and the measured γ-decay probability ratios.

doi: 10.1103/PhysRevC.94.015804
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset32732. Data from this article have been entered in the XUNDL database. For more information, click here.