NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = X.Y.Li Found 24 matches. 2024NA12 Phys.Rev. C 109, 045808 (2024) W.Nan, Y.P.Shen, B.Guo, Z.H.Li, Y.J.Li, D.Y.Pang, J.Su, S.Q.Yan, Q.W.Fan, J.C.Liu, C.Chen, X.Y.Li, G.Lian, T.L.Ma, W.K.Nan, Y.B.Wang, S.Zeng, H.Zhang, W.P.Liu New determination of the astrophysical SE1 factor of the 12C(α, γ)16O reaction via the 12C(11B, 7Li)16O transfer reaction
doi: 10.1103/PhysRevC.109.045808
2023LI48 Nucl.Phys. A1040, 122761 (2023) Spin-orbit amplitudes for decays with arbitrary spin
doi: 10.1016/j.nuclphysa.2023.122761
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
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
2022LI47 Phys.Rev. C 106, 025807 (2022) X.Y.Li, B.Guo, Z.H.Li, Y.J.Li, J.Su, D.Y.Pang, J.J.He, S.Q.Yan, Q.W.Fan, J.C.Liu, L.Gan, Z.Y.Han, E.T.Li, G.Lian, Y.P.Shen, Y.B.Wang, S.Zeng, W.P.Liu Astrophysical 15N(n, γ)16N reaction rate from precision measurement of the 15N(d, p)16N angular distributions NUCLEAR REACTIONS 15N(d, p), (d, d), E=15 MeV; measured particle spectra, σ(θ) using Q3D magnetic spectrograph at CIAE's HI-13 tandem accelerator facility. 16N; deduced levels, J, π, configurations, spectroscopic factors for ground and first three excited states. DWBA and ADWA analysis. 15N(n, γ), T=0.01-10 GK; deduced astrophysical reaction rates; calculated σ(E). Comparison with previous experimental results, and with OXBASH shell-model predictions.
doi: 10.1103/PhysRevC.106.025807
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
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
2021YA29 Astrophys.J. 919, 84 (2021) S.Q.Yan, X.Y.Li, K.Nishio, M.Lugaro, Z.H.Li, H.Makii, M.Pignatari, Y.B.Wang, R.Orlandi, K.Hirose The 59Fe(n, γ)60Fe Cross Section from the Surrogate Ratio Method and Its Effect on the 60Fe Nucleosynthesis NUCLEAR REACTIONS 56,58Fe(18O, 16O), E=103 MeV; measured reaction products, Eγ, Iγ; deduced σ, Maxwellian-averaged σ. Comparison with TALYS calculations.
doi: 10.3847/1538-4357/ac12ce
2021ZH46 Chin.Phys.C 48, 084108 (2021) H.Zhang, Z.i-H.Li, J.Su, Y.-J.Li, C.Chen, L.Zhang, F.-Q.Cao, Y.-P.Shen, W.Nan, W.-K.Nan, X.-Y.Li, L.-H.Chen, G.Lian, B.-Q.Cui, B.Guo, W.-P.Liu Direct measurement of the resonance strengths and branching ratios of low-energy (p, γ) reactions on Mg isotopes NUCLEAR REACTIONS 24,25,26Mg(p, γ), E=220-400 keV; measured reaction products, Eγ, Iγ; deduced γ-ray energies, yields, resonances, branching ratios, resonance strengths. JUNA experiment, comparison with NACRE data.
doi: 10.1088/1674-1137/ac06aa
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
2020GA03 Phys.Rev. C 101, 014612 (2020) L.Gan, H.B.Sun, Z.H.Li, S.P.Hu, Y.J.Li, J.Su, B.Guo, S.Q.Yan, Y.B.Wang, S.Zeng, Z.Y.Han, X.Y.Li, D.H.Li, T.L.Ma, Y.P.Shen, Y.Su, E.T.Li, W.P.Liu Experimental study of the spectroscopic factors of 116-125Sn NUCLEAR REACTIONS 116,118,120,122,124Sn(p, d), E=18.0 MeV; 116,118,120,122,124Sn(d, p), E=12.0 MeV; measured E(p), I(p), E(d), I(d), σ(θ) using the high-precision Q3D magnetic spectrograph at the CIAE-Beijing HI-13 tandem accelerator. 115,117,119,121,123,125Sn; deduced levels, L-transfers, J, π, spectroscopic factors (SFs). DWBA analysis of σ(θ) data and extraction of the neutron spectroscopic factors using two different sets of systematic optical potential parameters. Comparison with previous experimental data. Proposed a linear formula to relate SFs with S(n).
doi: 10.1103/PhysRevC.101.014612
2020LI17 Chin.Phys.C 44, 074001 (2020) X.-Y.Li, B.Guo, Z.-H.Li, W.-P.Liu Astrophysical 22Mg(p, γ)23Al reaction rates from asymptotic normalization coefficient of 23Ne → 22Ne + n RADIOACTIVITY 23Ne(n); analyzed available data; calculated squared neutron asymptotic normalization coefficients (ANCs) from the experimental differential cross-sections of the 22Ne(d, p) reaction through the ADWA and CDCC analysis.
doi: 10.1088/1674-1137/44/7/074001
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
2020SH09 Phys.Rev.Lett. 124, 162701 (2020) Y.P.Shen, B.Guo, R.J.deBoer, Z.H.Li, Y.J.Li, X.D.Tang, D.Y.Pang, S.Adhikari, C.Basu, J.Su, S.Q.Yan, Q.W.Fan, J.C.Liu, C.Chen, Z.Y.Han, X.Y.Li, G.Lian, T.L.Ma, W.Nan, W.K.Nan, Y.B.Wang, S.Zeng, H.Zhang, W.P.Liu Constraining the External Capture to the 16O ground State and the E2 S Factor of the 12C(α, γ)16O reaction NUCLEAR REACTIONS 12C(11B, 7Li)16O, E=50 MeV; measured reaction products; deduced σ(θ), the ground state asymptotic normalization coefficients, S-factors. Comparison with available data.
doi: 10.1103/PhysRevLett.124.162701
2019MA31 Nucl.Phys. A986, 26 (2019) T.L.Ma, B.Guo, Z.H.Li, Y.J.Li, D.Y.Pang, Y.L.Han, Y.P.Shen, J.Su, J.C.Liu, Q.W.Fan, Z.Y.Han, X.Y.Li, G.Lian, Y.Su, Y.B.Wang, S.Q.Yan, S.Zeng, W.P.Liu Precision measurement of the angular distribution for the 16O(d, p)17O transfer reaction to the ground state of 17O NUCLEAR REACTIONS 16O(d, p)17O, E=15 MeV; measured Ep, Ip(θ); deduced σ(θ) for reactions to 17O gs, spectroscopic factors, ANC; calculated σ(θ) for reactions to 17O gs using DWBA, ADWA (Adiabatic DWBA) and Continuum Discretized Coupled Channel (CDCC) vs radius parameter of Woods-Saxon potential with the same optical potential parameters in ADWA and CDCC. SF and ANC for 17O compared with published results in heavy ion transfer and with shell model calculations.
doi: 10.1016/j.nuclphysa.2019.03.004
2019SH11 Phys.Rev. C 99, 025805 (2019) Y.P.Shen, B.Guo, Z.H.Li, Y.J.Li, D.Y.Pang, S.Adhikari, Z.D.An, J.Su, S.Q.Yan, X.C.Du, Q.W.Fan, L.Gan, Z.Y.Han, D.H.Li, E.T.Li, X.Y.Li, G.Lian, J.C.Liu, T.L.Ma, C.J.Pei, Y.Su, Y.B.Wang, S.Zeng, Y.Zhou, W.P.Liu Astrophysical SE2 factor of the 12C (α, γ)16O reaction through the 12C(11B, 7Li)16O transfer reaction NUCLEAR REACTIONS 12C(11B, 7Li), (11B, 11B), E=50 MeV; 16O(7Li, 7Li), E=26 MeV; measured charged-particle spectra, differential σ(θ) using the Q3D magnetic spectrograph at the HI-13 tandem accelerator of the CIAE-Beijing. 12C(α, γ), E(cm)<5 MeV; deduced astrophysical SE2(300) factor of the ground state. 16O; deduced asymptotic normalization coefficient (ANC) and reduced α width of the 6.917-MeV level from finite-range distorted wave Born approximation (FRDWBA) and coupled-reaction-channel (CRC) analysis using FRESCO code. Comparison with previous experimental values, and with theoretical model predictions. R-matrix analysis of scattering data.
doi: 10.1103/PhysRevC.99.025805
2019SH37 Phys.Lett. B 797, 134820 (2019) Y.P.Shen, B.Guo, T.L.Ma, D.Y.Pang, D.D.Ni, Z.Z.Ren, Y.J.Li, Z.D.An, J.Su, J.C.Liu, Q.W.Fan, Z.Y.Han, X.Y.Li, Z.H.Li, G.Lian, Y.Su, Y.B.Wang, S.Q.Yan, S.Zeng, W.P.Liu First experimental constraint of the spectroscopic amplitudes for the α-cluster in the 11B ground state NUCLEAR REACTIONS 7Li(6Li, d), E=24 MeV; measured reaction products; deduced spectroscopic amplitudes (SA) for the α-cluster in the 11B ground state. Comparison with available data.
doi: 10.1016/j.physletb.2019.134820
2018GA19 Phys.Rev. C 97, 064614 (2018) L.Gan, H.B.Sun, Z.H.Li, Y.J.Li, J.Su, B.Guo, S.Q.Yan, Y.B.Wang, S.Zeng, Z.Y.Han, X.Y.Li, D.H.Li, T.L.Ma, Y.P.Shen, Y.Su, E.T.Li, S.P.Hu, W.P.Liu Experimental study of the spectroscopic factors of 90-97Zr NUCLEAR REACTIONS 90,92,94,96Zr(12C, 12C), (12C, 13C), E=66 MeV; 90,92,94,96Zr(13C, 13C), (13C, 12C), E=64 MeV; measured particle spectra, differential σ(θ) using Q3D magnetic spectrograph at the HI-13 tandem accelerator facility of the CIAE, Beijing; deduced neutron spectroscopic factors using distorted-wave Born approximation (DWBA) calculations. Comparison of spectroscopic results with previous experiments. Relevance to neutron capture reactions in s process for synthesis of heavy elements.
doi: 10.1103/PhysRevC.97.064614
2018LI38 Chin.Phys.Lett. 35, 072301 (2018) Y.-M.Liu, J.-B.Lu, X.-Y.Li, X.Xu, R.He, R.-Z.Zheng, G.-D.Wei Theoretical Prediction of Diamond Betavoltaic Batteries Performance Using 63Ni
doi: 10.1088/0256-307X/35/7/072301
2018MA06 Phys.Rev. C 97, 014305 (2018) K.Y.Ma, J.B.Lu, Z.Zhang, J.Q.Liu, D.Yang, Y.M.Liu, X.Xu, X.Y.Li, Y.Z.Liu, X.G.Wu, Y.Zheng, C.B.Li Candidate chiral doublet bands in 138Pm NUCLEAR REACTIONS 124Te(19F, 5n), E=105 MeV from HI-13 tandem accelerator at CIAE, Beijing; measured Eγ, Iγ, γγ-coin, γγ(θ)(DCO) using an array of ten Compton-suppressed HPGe, one HPGe planar and one clover Ge detectors. 138Pm; deduced high-spin levels, J, π, chiral doublet band, energy staggering, alignments, configuration, B(M1)/B(E2) ratio. Cranked shell model calculations for quasiproton and quasineutron Routhians, and total Routhian surface (TRS) in (β, γ) plane. Systematics of energy staggering in chiral doublet bands in 120,122,124,126,128,130,132Cs, 124,126,128,130,132,134La, 126,128,130,132,134,136Pr, 134,136,138Pm.
doi: 10.1103/PhysRevC.97.014305
2017MA04 Eur.Phys.J. A 53, 10 (2017) K.Y.Ma, J.B.Lu, X.Xu, Y.M.Liu, Z.Zhang, X.Y.Li, D.Yang, Y.Z.Liu, X.G.Wu, C.Y.He, Y.Zheng, C.B.Li Structure of a positive-parity band in 130Pr NUCLEAR REACTIONS 99Ru(35Cl, 2n2p), E=151 MeV; measured Eγ, Iγ, γγ-coin using nine Compton-suppressed HPGe, two planar HPGe and one clover detector; deduced γ transitions, levels, J, π, rotational bands, high-spin states, transition multipolarity, possible interpretation of the side band.
doi: 10.1140/epja/i2017-12204-y
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
2012WA07 Int.J.Mod.Phys. E21, 1250009 (2012) Nucleon effective mass in cold dense matter
doi: 10.1142/S0218301312500097
2009LI40 Phys.Rev. C 80, 034909 (2009) X.-y.Li, X.-f.Lu, B.Wang, W.-m.Sun, H.-s.Zong Properties of cold dense nuclear matter based on a nonperturbative approach inspired by chiral perturbation theory
doi: 10.1103/PhysRevC.80.034909
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