NSR Query Results


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NSR database version of April 11, 2024.

Search: Author = L.C.He

Found 5 matches.

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2023LI11      Phys.Rev. C 107, 024609 (2023)

G.-S.Li, J.Su, B.-H.Sun, S.Terashima, J.-W.Zhao, X.-D.Xu, J.-C.Zhang, G.Guo, L.-C.He, W.-P.Lin, W.-J.Lin, C.-Y.Liu, C.-G.Lu, B.Mei, Z.-Y.Sun, I.Tanihata, M.Wang, F.Wang, S.T.Wang, X.-L.Wei, J.Wang, J.-Y.Xu, J.-R.Liu, M.-X.Zhang, Y.Zheng, L.-H.Zhu, X.-H.Zhang

New measurement of the elemental fragmentation cross sections of 218 MeV/nucleon 28Si on a carbon target

NUCLEAR REACTIONS 12C(28Si, X), E=218 MeV/nucleon; measured reaction products, time-of-flight; deduced charge changing σ, elemental fragmentation σ (EFCSs) with charge changes 1-6. Comparison to the previous measurements and to the predictions from the models EPAX2, EPAX3, FRACS, ABRABLA07, NUCFRG2, and IQMD coupled with GEMINI (IQMD+GEMINI). Particle identification by means of MWPC and MUSIC detectors. Beam of 28Si produced from 9Be(40Ar, X), E=320 MeV/nucleon at Heavy Ion Research Facility (HIRFL-CSR, Lanzhou).

doi: 10.1103/PhysRevC.107.024609
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2021CH36      Astrophys.J. 915, 78 (2021)

H.Cheng, B.-H.Sun, L.-H.Zhu, M.Kusakabe, Y.Zheng, L.C.He, T.Kajino, Z.-M.Niu, T.-X.Li, C.-B.Li, D.-X.Wang, M.Wang, G.-S.Li, K.Wang, L.Song, G.Guo, Z.-Y.Huang, X.-L.Wei, F.-W.Zhao, X.-G.Wu, Y.Abulikemu, J.-C.Liu, P.Fan

Measurements of 160Dy(p, γ) at Energies Relevant for the Astrophysical γ Process

NUCLEAR REACTIONS 160Dy(p, γ), 161Dy(p, n), E=3.4-7 MeV; measured reaction products, Eγ, Iγ; deduced σ, S-factor, astrophysical reaction rates. Comparison with TALYS, NON-SMOKER calculations.

doi: 10.3847/1538-4357/ac00b1
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2020WA07      Eur.Phys.J. A 56, 31 (2020)

M.Wang, W.J.Sun, B.H.Sun, J.Li, L.H.Zhu, Y.Zheng, G.L.Zhang, L.C.He, W.W.Qu, F.Wang, T.F.Wang, C.Xiong, C.Y.He, G.S.Li, J.L.Wang, X.G.Wu, S.H.Yao, C.B.Li, H.W.Li, S.P.Hu, J.J.Liu

The ΔI = 2 bands in 109In: possible antimagnetic rotation

NUCLEAR REACTIONS 100Mo(14N, 5n), E=78 MeV; measured Eγ, Iγ, γγ-coin, γγ(θ)(DCO) using two low-energy photon detectors and nine BGO-Compton-suppressed HPGe detectors at CIAE-Beijing. 109In; deduced levels, J, π, multipolarities, anti-magnetic rotational band, alignments, configurations. Comparison with calculations using titled axis cranking calculation in the framework of covariant density function theory (TAC-CDFT), and with previous experimental results. Systematics of bands based on πg7/2 orbital in 107,109,111,113In. See also 2018Wa15, a related experiment from the same laboratory.

doi: 10.1140/epja/s10050-020-00039-6
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Data from this article have been entered in the XUNDL database. For more information, click here.


2018WA15      Phys.Rev. C 98, 014304 (2018), Erratum Phys.Rev. C 102, 069903 (2020)

M.Wang, Y.Y.Wang, L.H.Zhu, B.H.Sun, G.L.Zhang, L.C.He, W.W.Qu, F.Wang, T.F.Wang, Y.Y.Chen, C.Xiong, J.Zhang, J.M.Zhang, Y.Zheng, C.Y.He, G.S.Li, J.L.Wang, X.G.Wu, S.H.Yao, C.B.Li, H.W.Li, S.P.Hu, J.J.Liu

New high-spin structure and possible chirality in 109In

NUCLEAR REACTIONS 100Mo(14N, 5n), E=78 MeV; measured Eγ, Iγ, γγ-coin, γγ(θ)(DCO) using two low-energy photon detectors and nine BGO-Compton-suppressed HPGe detectors at CIAE-Beijing. 109In; deduced levels, J, π, multipolarities, bands, alignments, configurations, and possible chiral partner bands. Comparison with calculations using titled axis cranking calculation in the framework of covariant density function theory (TAC-CDFT), and with previous experimental results. Systematics of yrast states in 103,105,107,109,111,113In.

doi: 10.1103/PhysRevC.98.014304
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2017HE09      Chin.Phys.C 41, 044003 (2017)

L.-C.He, Y.Zheng, L.-H.Zhu, H.-L.Ma, X.-G.Wu, C.-Y.He, G.-S.Li, L.-L.Wang, X.Hao, Y.Liu, X.-Q.Li, B.Pan, Z.-Y.Li, H.-B.Ding

Collective states and shape competition in 126Te

NUCLEAR REACTIONS 124Sn(7Li, 4np)126Te, E=48 MeV; measured reaction products, Eγ, Iγ; deduced energies, relative intensities, directional correlation of oriented states ratios, and initial and final state J, π of γ-rays. Comparison with theoretical calculations.

doi: 10.1088/1674-1137/41/4/044003
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Data from this article have been entered in the XUNDL database. For more information, click here.


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