Neutron production in neutron-induced reactions at 96 MeV on<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow /><mml:mn>56</mml:mn></mml:msup></mml:math>Fe and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mrow /><mml:mn>208</mml:mn></mml:msup></mml:math>Pb

García, Ignacio Cristobal; Lecolley, J.F.; Lecolley, F. R.; Blidéanu, V.; Ban, G.; Fontbonne, J.M.; Itis, G.; Lecouey, J. L.; Lefort, T.; Marie, N.; Steckmeyer, J.C.; Brun, C. Le; Blomgren, J.; Johansson, Cecilia; Klug, J.; Öhrn, Angelica; Mermod, P.; Olsson, N.; Pomp, Stephan; Österlund, Michael; Tippawan, U.; Prokofiev, Alexander V.; Nadel‐Turoński, P.; Fallot, M.; Foucher, Y.; Guertin, Arnaud; Haddad, Férid; Vatre, M.

doi:10.1103/physrevc.84.044619

Cited by 3 publications

(5 citation statements)

References 29 publications

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“…We note that the charge radii of the Zr isotopes obtained by the present models show the large difference as displayed in Fig. 2, whereas the rms radii of the point-matter densities are similar to each other: The RMF (HF + BCS) model gives 4.111, 4.251, 4.560, and 4.665 fm (4.137, 4.244, 4.516, and 4.698 fm) for rms radii of the point-matter densities of the 80 Zr, 90 Zr, 100 Zr, and 110 Zr nuclei, respectively. Here we compared our results for the selected nuclei.…”

Section: Comparison Between Rmf and Hf + Bcs Modelssupporting

confidence: 56%

“…4. Point-neutron, proton, and matter density distributions of (a) 80 Zr, (b) 90 Zr, (c) 100 Zr, and (d) 110 Zr.…”

Section: Comparison Between Rmf and Hf + Bcs Modelsmentioning

confidence: 99%

“…We calculate the SF potentials for the pA and nA systems with Z T = 6-92 and A T = 10-276 target nuclei at E = 50, 60,70,80,90,100,120,140,160,180,200,300, and 400 MeV. The parameter sets at other incident energies between 50 and 400 MeV are obtained by the spline interpolation.…”

Section: Functional Form Of Microscopic Global Optical Potentialmentioning

confidence: 99%

“…(1) Z T = 6-20: 12 C, 16 O, 20 Ne, 24 Mg, 28 Si, 32 S, 40 Ar, 40 Ca, 42 Ca, 44 Ca, and 48 Ca; (2) Z T = 22-28: 46 Ti, 48 Ti, 50 Ti, 50 Cr, 52 Cr, 54 Cr 54 Fe, 56 Fe, 58 Ni, 60 Ni, 62 Ni, and 64 Ni; (3) Z T = 40-68: 90 Zr, 98 Mo, 100 Mo, 144 Sm, 148 Sm, 150 Sm, 152 Sm, 154 Sm, 160 Gd, 164 Dy, 166 Er, and 168 Er; (4) Z T = 70-92: 172 Yb, 174 Yb, 176 Yb, 178 Hf, 180 Hf, 182 W, 184 W, 192 Os, 208 Pb, 232 Th, and 238 U.…”

Section: Proton-nucleus Elastic-scattering Cross Sections At 65 Mevmentioning

confidence: 99%

“…In addition, we show some results of the proton elastic-scattering cross section and the analyzing power involving the unstable nuclei far from the stability line. We select 48 S, 100 Zr, and 110 Zr because the two mean-field models give the quite different 48 Ti, 50 Ti, 50 Cr, 54 Fe, 56 Fe, 58 Ni, 60 Ni, 62 Ni, 66 Zn, 68 Zn, 74 Se, 76 Se, 78 Se, 80 Se, and 82 Se systems at E p = 51.9-333 MeV in the Rutherford ratio; (b) analyzing power of p + 54 Fe, 56 Fe, 58 Ni, and 60 Ni systems at E p = 60. 108 Pd, 110 Pd, 112 Cd, and 116 Sn systems in the Rutherford ratio at E p = 51-61.4 MeV.…”

Section: Proton-nucleus Elastic-scattering Cross Sections For Unstablmentioning

confidence: 99%

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Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

et al. 2019

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We provide a microscopic global optical potential (MGOP) for nucleon-nucleus (NA) systems in a wide range of nuclear mass numbers (A = 10-276) and incident energies (E = 50-400 MeV). The potential is microscopically constructed based on a single-folding (SF) model with the complex G-matrix interaction. The nuclear densities used in the SF model are generated, in a nonempirical way, from two kinds of microscopic mean-field models: the relativistic-mean-field (RMF) and Skyrme-Hartree-Fock + BCS (HF+BCS) models. We calculate the NA potentials for more than 1000 even-even nuclei with atomic number Z = 6-92, involving proton-and neutron-rich unstable nuclei. We confirm that both the MGOP models well reproduce the available experimental data of the total reaction cross sections, the total neutron cross sections, the elastic-scattering cross sections, the analyzing power, and the spin-rotation function Q. We also calculate the proton scattering cross sections of 22 O, 24 O, and 56 Ni targets to compare the experimental data and then the cross sections for unknown 48 S, 100 Zr, and 110 Zr are presented for future measurements. For the sake of convenience, the real and imaginary parts of the central and spin-orbit components of the NA potentials are respectively represented in a linear combination of 12-range Gaussians. They are provided on the website [http://www2.yukawa.kyoto-u.ac.jp/∼ takenori.furumoto/] with a program source file for reconstructing the MGOP.

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Section: Comparison Between Rmf and Hf + Bcs Modelssupporting

confidence: 56%

“…4. Point-neutron, proton, and matter density distributions of (a) 80 Zr, (b) 90 Zr, (c) 100 Zr, and (d) 110 Zr.…”

Section: Comparison Between Rmf and Hf + Bcs Modelsmentioning

confidence: 99%

Section: Functional Form Of Microscopic Global Optical Potentialmentioning

confidence: 99%

Section: Proton-nucleus Elastic-scattering Cross Sections At 65 Mevmentioning

confidence: 99%

Section: Proton-nucleus Elastic-scattering Cross Sections For Unstablmentioning

confidence: 99%

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Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

et al. 2019

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Measurement of neutron-induced proton-production energy spectra with NE213 scintillator

Kajimoto¹,

Shigyo²,

Ishibashi³

et al. 2012

Radiation Measurements

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Study the Structure and Optical Properties of GNPs Doped WO₃/PS by Spray Pyrolysis Deposition (SPD)

Hasan

Al‐Samarai

Obaid

et al. 2021

IOP Conf. Ser.: Mater. Sci. Eng.

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In this studied gold (Au) nanoparticles doped tungsten oxide (WO3) thin film was deposited on porous silicon (PS) substrate at the substrate temperature of 250°C by spray pyrolysis deposition method, with different Au doping concentration of (0, 1, 3, and 5%). The gold nanoparticles GNPs were prepared by using normal atmospheric air cold plasma. All films were annealed at 500°C for 1h. The X-ray diffraction peaks indicated that all films are polycrystalline with a hexagonal structure. The surface morphology was studied by AFM. The average grain size for pure thin film WO3 was about 61 nm, and it decreased to be about 43.2 nm with increases the doping ratios for the film deposited at 5% of Au. FESEM image all doped and undoped films showed homogenous pattern structure on the porous silicon. The thickness of films was obtained from the cross-section of the FESEM, which was 323±5 nm. A blue-shifted showed based on the photolumenses (PL) peak position calculated of WO3 as doping ratio increased, the bandgap for Au: WO3 films lies between (2.85 to 3.02) eV.

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Neutron production in neutron-induced reactions at 96 MeV on56Fe and208Pb

Cited by 3 publications

References 29 publications

Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

Measurement of neutron-induced proton-production energy spectra with NE213 scintillator

Study the Structure and Optical Properties of GNPs Doped WO₃/PS by Spray Pyrolysis Deposition (SPD)

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Neutron production in neutron-induced reactions at 96 MeV on56Fe and208Pb

Cited by 3 publications

References 29 publications

Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

Microscopic global optical potential for nucleon-nucleus systems in the energy range 50–400 MeV

Measurement of neutron-induced proton-production energy spectra with NE213 scintillator

Study the Structure and Optical Properties of GNPs Doped WO3/PS by Spray Pyrolysis Deposition (SPD)

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Product

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Study the Structure and Optical Properties of GNPs Doped WO₃/PS by Spray Pyrolysis Deposition (SPD)