NSR Query Results

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NSR database version of April 11, 2024.

Search: Author = H.Lan

Found 6 matches.

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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
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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
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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
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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
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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
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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
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Note: The following list of authors and aliases matches the search parameter H.Lan: , H.Y.LAN