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NSR database version of April 11, 2024.

Search: Author = L.H.Wang

Found 8 matches.

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2024YA05      Chin.Phys.C 48, 034001 (2024)

G.Yang, F.-F.Duan, K.Wang, Y.-Y.Yang, Zh.-Y.Sun, V.Guimaraes, D.-Y.Pang, W.-D.Chen, L.Jin, Sh.-W.Xu, J.-B.Ma, P.Ma, Zh.Bai, L.-H.Wang, Q.Liu, H.-J.Ong, B.-F.Lv, S.Guo, M.K.Raju, X.-H.Wang, R.-H.Li, Y.-H.Zhang, X.-H.Zhou, Zh.-G.Hu, H.-Sh.Xu

Elastic scattering of 13C and 14C isotopes on a 208Pb target at energies of approximately five times the Coulomb barriers

NUCLEAR REACTIONS 208Pb(13C, 13C), E=340 MeV; 208Pb(14C, 14C), E=294, 342 MeV; measured reaction products; deduced σ(θ) within the optical model and continuum-discretized coupled-channels (CDCC) framework. Comparison with available data. The Heavy-Ion Research Facility in Lanzhou (HIRFL), the National Laboratory of Heavy Ion Research of the Institute of Modern Physics.

doi: 10.1088/1674-1137/ad1678
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2023WA05      Phys.Rev.Lett. 130, 092701 (2023)

L.H.Wang, J.Su, Y.P.Shen, J.J.He, M.Lugaro, B.Szanyi, A.I.Karakas, L.Y.Zhang, X.Y.Li, B.Guo, G.Lian, Z.H.Li, Y.B.Wang, L.H.Chen, B.Q.Cui, X.D.Tang, B.S.Gao, Q.Wu, L.T.Sun, S.Wang, Y.D.Sheng, Y.J.Chen, H.Zhang, Z.M.Li, L.Y.Song, X.Z.Jiang, W.Nan, W.K.Nan, L.Zhang, F.Q.Cao, T.Y.Jiao, L.H.Ru, J.P.Cheng, M.Wiescher, W.P.Liu

Measurement of the 18O(α, γ)22Ne Reaction Rate at JUNA and Its Impact on Probing the Origin of SiC Grains

NUCLEAR REACTIONS 18O(α, γ), E=470-787 keV; measured reaction products, Eγ, Iγ; deduced thick target yields, resonance energies and resonance strengths, total reaction rates. Comparison with available data. The Jinping Underground Nuclear Astrophysics experimental facility (JUNA).

doi: 10.1103/PhysRevLett.130.092701
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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.


2022WA02      Nucl.Instrum.Methods Phys.Res. B512, 49 (2022)

L.H.Wang, Y.P.Shen, J.Su, X.Y.Li, W.Q.Yan, J.J.He, L.Y.Zhang, B.Liao, Y.F.Wu, Y.D.Sheng, Z.M.Li, Y.J.Chen, L.Y.Song, X.Z.Jiang, G.Lian, W.Nan, W.K.Nan, L.Zhang, F.Q.Cao, C.Chen, N.Song, H.Zhang, W.P.Liu

Development of irradiation-resistant enriched 12C targets for astrophysical 12C(α, γ)16O reaction measurements

NUCLEAR REACTIONS 12C(p, γ), E=370 keV; 12C(p, α), E=740 keV; measured reaction products, Eγ, Iγ; deduced yields. The China JinPing underground Laboratory (CJPL).

doi: 10.1016/j.nimb.2021.11.020
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2022ZH67      Phys.Rev. C 106, 055803 (2022)

L.Y.Zhang, J.Su, J.J.He, R.J.deBoer, D.Kahl, M.Wiescher, D.Odell, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, B.Guo, X.D.Tang, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, J.P.Cheng, W.P.Liu

Direct measurement of the astrophysical 19F(p, αγ)16O reaction in a deep-underground laboratory

NUCLEAR REACTIONS 19F(p, αγ), E(cm)=72.4-344 keV; measured Eγ, Iγ; deduced astrophysical S-factor, thermonuclear astrophysical reaction rates (range 0.05–1 GK), contributions from different channels. R-matrix analysis with AZURE2 together with a MCMC Bayesian uncertainty estimation. Comparison to other experimental data. 4π BGO γ-array with proton beam from JUNA accelerator at China JinPing underground Laboratory (CJPL).

doi: 10.1103/PhysRevC.106.055803
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Data from this article have been entered in the XUNDL database. For more information, click here.


2021ZH53      Phys.Rev.Lett. 127, 152702 (2021)

L.Y.Zhang, J.Su, J.J.He, M.Wiescher, R.J.deBoer, D.Kahl, Y.J.Chen, X.Y.Li, J.G.Wang, L.Zhang, F.Q.Cao, H.Zhang, Z.C.Zhang, T.Y.Jiao, Y.D.Sheng, L.H.Wang, L.Y.Song, X.Z.Jiang, Z.M.Li, E.T.Li, S.Wang, G.Lian, Z.H.Li, X.D.Tang, H.W.Zhao, L.T.Sun, Q.Wu, J.Q.Li, B.Q.Cui, L.H.Chen, R.G.Ma, B.Guo, S.W.Xu, J.Y.Li, N.C.Qi, W.L.Sun, X.Y.Guo, P.Zhang, Y.H.Chen, Y.Zhou, J.F.Zhou, J.R.He, C.S.Shang, M.C.Li, X.H.Zhou, Y.H.Zhang, F.S.Zhang, Z.G.Hu, H.S.Xu, J.P.Chen, W.P.Liu

Direct Measurement of the Astrophysical 19F(p, αγ)16O Reaction in the Deepest Operational Underground Laboratory

NUCLEAR REACTIONS 19F(p, α), E(cm)=72.4-188.8 keV; measured reaction products, Eγ, Iγ; deduced yields, S-factors, reaction rates. The China Jinping Underground Laboratory (CJPL), JUNA accelerator.

doi: 10.1103/physrevlett.127.152702
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2019HU16      Chin.J.Phys.(Taiwan) 60, 88 (2019)

L.-D.Huo, L.-H.Wang, J.-H.Zhu, H.-L.Li, J.-S.Li, S.Kodaira, N.Yasuda, D.-H.Zhang

The total charge-changing cross sections and the partial cross sections of 56Fe fragmentation on Al, C and CH2 targets

NUCLEAR REACTIONS C, 27Al(56Fe, X), E=496 MeV/nucleon; measured reaction products; deduced total charge-changing σ and the partial σ.

doi: 10.1016/j.cjph.2019.04.022
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2017ZH11      J.Phys.(London) G44, 045110 (2017)

H.F.Zhang, L.H.Wang, J.P.Yin, P.H.Chen, H.F.Zhang

Performance of the Levenberg-Marquardt neural network approach in nuclear mass prediction

NUCLEAR STRUCTURE A<270; calculated binding energies, rms radii, one-neutron and two-neutron separation energies, masses. FRDM, WS4, Bhagwat, LMNN models. Comparison with available data.

doi: 10.1088/1361-6471/aa5d78
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