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NSR database version of April 27, 2024.

Search: Author = Z.C.Zhu

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2024SH13      Nucl.Instrum.Methods Phys.Res. A1062, 169222 (2024)

X.-M.Shi, G.-L.Wang, K.-J.Luo, X.-X.Li, Zh.-Ch.Zhu, W.Luo

Geant4 development for actinides photofission simulation

NUCLEAR REACTIONS ²³²Th(γ, F), E=16 MeV; ²³⁵U(γ, F), E=13 MeV; ²³⁸U(γ, F), E=17.2 MeV; ²⁴²Pu(γ, F), E=20 MeV; calculated mass yield distri'butions (MYD), the isobaric charge distributions (ICD), and the multiplicity and spectral distributions with the Geant4 simulations. comparison with the available experimental data.

doi: 10.1016/j.nima.2024.169222
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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, ^{88,89,90,91,92}Kr, ^{91,92,93,94,95}Rb, ^{93,94,95,96,97}Sr, ^{96,97,98,99,100}Y, ^{98,99,100,101,102}Zr, ^{101,102,103,104}Nb, ^104,105Mo, ¹³⁰Sn, ^{130,131,132,133}Sb, ^{132,133,134,135,136}Te; 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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2009HU20      Chin.Phys.C 33, Supplement 1, 193 (2009)

W.-X.Huang, J.-Y.Wang, Y.Wang, Y.-L.Tian, Z.-C.Zhu, H.-S.Xu, G.-Q.Xiao

Simulation of the Lanzhou Penning Trap LPT

doi: 10.1088/1674-1137/33/S1/062
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