NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = H.Lan Found 6 matches. 2024WA08 Nucl.Phys. A1043, 122834 (2024) M.Z.Wang, D.Wu, H.Y.Lan, J.Y.Zhang, J.X.Liu, H.G.Lu, J.F.Lv, X.Z.Wu, H.Zhang, J.Cai, Q.Y.Ma, Y.H.Xia, Z.N.Wang, Z.Y.Yang, X.L.Xu, Y.X.Geng, Y.Y.Zhao, H.R.Wang, F.L.Liu, J.Q.Yu, K.J.Luo, W.Luo, X.Q.Yan Cross section measurements of 27Al(γ, x)24Na reactions as monitors for laser-driven bremsstrahlung γ-ray NUCLEAR REACTIONS 27Al(γ, X)24Na, E ∼ 78, 103, 135; measured reaction products, Eγ, Iγ; deduced γ-ray energies, σ. Comparison with TALYS 1.9 calculations, experimental data. The 200 TW laser facility in the Compact Laser Plasma Accelerator (CLAPA) Laboratory, Peking University.
doi: 10.1016/j.nuclphysa.2024.122834
2023AN14 Sci. Rep. 13, 12657 (2023) Z.An, W.Qiu, W.Jiang, G.Yang, X.Li, Z.Liao, Z.Zhuang, X.Zhang, S.Chen, C.Guo, E.Xiao, X.Fang, X.Li, H.Wang, X.Hu, Bi.Jiang, W.Shen, J.Wang, J.Ren, X.Ruan, D.Wang, S.-Y.Zhang, W.Luo, Z.Zhu, H.Lan, Z.Cao, X.Ma, Y.Liu, P.Wang, Y.Yang, P.Su, X.Deng, W.He, Y.Ma, C.Ma, Y.Wang, P.He, R.Tang, T.Zhou, J.Wang, H.Yi, Y.Zhang, Y.Chen, R.Fan, K.Gao, Q.Li, K.Sun, Z.Tan, M.Gu, H.Jing, J.Tang Measurement of the 181Ta(n, γ) cross sections up to stellar s-process temperatures at the CSNS Back-n NUCLEAR REACTIONS 181Ta(n, γ), E=0.001-800 keV; measured reaction products, En, In, TOF; deduced σ, resonance parameters using the R-Matrix code SAMMY, Maxwellian average cross sections (MACS). Comparison with available data. The back-streaming white neutron facility (Back-n) of China spallation neutron source (CSNS).
doi: 10.1038/s41598-023-39603-7
2022LA06 Phys.Rev. C 105, 044618 (2022) H.Y.Lan, W.Luo, Y.Xu, D.L.Balabanski, G.L.Guardo, M.La Cognata, D.Lattuada, C.Matei, R.G.Pizzone, T.Rauscher, J.L.Zhou Feasibility of studying astrophysically important charged-particle emission with the variable energy γ-ray system at the Extreme Light Infrastructure--Nuclear Physics facility NUCLEAR REACTIONS 29Si, 47Ti, 56Fe, 73Ge, 74Se, 84Sr, 91Zr, 95Mo, 96,98Ru, 102Pd, 106Cd, 115,117,119Sn, 132Ba, 143Nd(γ, p), (γ, np), E<30 MeV; 50V, 67Zn, 87Sr, 107Ag, 113,115In, 119Sn, 123,125Te, 149,154Sm, 155,156,157,158,160Gd, 208Pb(γ, α), (γ, nα), E<30 MeV; calculated inclusive and exclusive σ(E), population of the particular excited states, energy spectra of ejectiles. TALYS-1.9 calculations with various combinations of level densities, strength functions and optical potentials available in the code.Investigated the feasibility of studying the reactions of astrophysical interest with ELI-NP facility infrastructure. Simulated achievable yields.
doi: 10.1103/PhysRevC.105.044618
2022WA31 Chin.Phys.C 46, 084102 (2022) G.-L.Wang, H.-Y.Lan, X.-M.Shi, Z.-C.Zhu, W.Luo A general framework for describing photofission observables of actinides at an average excitation energy below 30 MeV NUCLEAR REACTIONS 232Th, 235,238U, 240Pu(γ, F), E<30 MeV; analyzed available data. 85Se, 87,88,89Br, 88,89,90,91,92Kr, 91,92,93,94,95Rb, 93,94,95,96,97Sr, 96,97,98,99,100Y, 98,99,100,101,102Zr, 101,102,103,104Nb, 104,105Mo, 130Sn, 130,131,132,133Sb, 132,133,134,135,136Te; calculated yields of photofission, neutron multiplicity and spectral distributions, nubar.
doi: 10.1088/1674-1137/ac6abc
2021PA03 Appl.Radiat.Isot. 168, 109534 (2021) W.t.Pan, T.Song, H.-y.Lan, Z.-g.Ma, J.-l.Zhang, Z.-c.Zhu, W.Luo Photo-excitation production of medically interesting isomers using intense γ-ray source NUCLEAR REACTIONS 103Rh, 113,115In, 176Lu(γ, γ'), E<30 MeV; calculated isomer production σ, specific activities, yields; deduced suitable decay properties for photo-excitation approach.
doi: 10.1016/j.apradiso.2020.109534
2018LA14 Phys.Rev. C 98, 054601 (2018) H.Y.Lan, Y.Xu, W.Luo, D.L.Balabanski, S.Goriely, M.La Cognata, C.Matei, A.Anzalone, S.Chesnevskaya, G.L.Guardo, D.Lattuada, R.G.Pizzone, S.Romano, C.Spitaleri, A.Taffara, A.Tumino, Z.C.Zhu Determination of the photodisintegration reaction rates involving charged particles: Systematic calculations and proposed measurements based on the facility for Extreme Light Infrastructure--Nuclear Physics NUCLEAR REACTIONS 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te(γ, p), E(cm)=8-20 MeV; 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te, 132Ba, 144Sm, 148Gd, 184Os(γ, α), E(cm)=6-20 MeV; calculated σ(E), proton and α-particle spectra and yields, Gamow windows at T9=2.5 and minimum required energies of the incident γ beam satisfying the measurable criteria of the minimum detectable limit and the particle identification. Z=10-100, N=10-160; calculated ratios of the (γ, p) and (γ, α) astrophysical reaction rates at T9=2.5 for 3000 targets of stable and proton-rich nuclei. Optical potential model calculations using Woods-Saxon and microscopic folding JLMB optical model potentials. Relevance to p-process nucleosynthesis, and the measurements of six (γ, p) and eight (γ, α) reactions based on the γ-beam facility and the Extreme Light Infrastructure Silicon Strip Array (ELISSA) for the detection of charged particles at ELI-NP, Bucharest facility.
doi: 10.1103/PhysRevC.98.054601
Back to query form Note: The following list of authors and aliases matches the search parameter H.Lan: , H.Y.LAN |