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NSR database version of April 27, 2024.

Search: Author = Q.B.Shen

Found 16 matches.

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2020CH17      Chin.Phys.C 44, 054109 (2020)

W.-D.Chen, H.-R.Guo, W.-L.Sun, T.Ye, Y.-J.Ying, Y.-L.Han, Q.B.Shen

Microscopic study of 7Li-nucleus potential

NUCLEAR REACTIONS 58Ni, 27Al, 65Cu, 89Y, 116Sn, 138Ba, 208Pb, 28Si, 13C(7Li, 7Li), E<300 MeV; analyzed available data. 7Li; calculated σ.

doi: 10.1088/1674-1137/44/5/054109
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2018XU12      Int.J.Mod.Phys. E27, 1850099 (2018)

Y.-Li.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

Global phenomenological optical model potentials for 8, 10, 11B projectiles

NUCLEAR REACTIONS 28,30Si, 40Ca, 58Ni, 208Pb, 209Bi(11B, 11B), E<100 MeV; 7Li, 9Be, 12C, 28Si, 58Ni, 208Pb(8B, 8B), E < 100 MeV; 16O, 28Si, 120Sn, 208Pb, 232Th(10B, 10B), E<100 MeV; analyzed available data for 11B; deduced global phenomenological optical model potential for 11B, calculated σ.

doi: 10.1142/S0218301318500994
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2016XU02      Int.J.Mod.Phys. E25, 1650013 (2016)

Y.-L.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

The neutron microscopic optical potential based on skyrme interaction

NUCLEAR REACTIONS 24Mg, 54,56Fe, 59Co, 90Zr, 93Nb, 92,96,98,100Mo, 120Sn, 206,208Pb(n, n), E=11 MeV; 12C, 16O, 23Na, 14N, 232Th, 235,238U, 239Pu(n, X), E=0.1-100 MeV; calculated σ(θ), σ. Comparison with experimental data.

doi: 10.1142/S0218301316500130
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2015XU04      Int.J.Mod.Phys. E24, 1550005 (2015)

Y.-L.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

Applicability of the systematic helium-3 potential for triton-nucleus reactions

NUCLEAR REACTIONS 28Si, 58Ni, 116Sn, 208Pb(t, t), (3He, 3He), E<60 MeV/nucleon; calculated σ; deduced optical model potential parameters. Comparison with available data.

doi: 10.1142/S0218301315500056
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2010GU01      Chin.Phys.Lett. 27, 012401 (2010)

H.-R.Guo, Y.-L.Han, Q.-B.Shen

A Microscopic Optical Potential for Deuteron

NUCLEAR REACTIONS 40Ca(d, X), (d, d), (d, d'), E=10-110 MeV; calculated microscopic optical potential for deuteron; deduced σ, σ(θ). Comparison with experimental data.

doi: 10.1088/0256-307X/27/1/012401
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2009SH31      Phys.Rev. C 80, 024604 (2009)

Q.-b.Shen, Y.-l.Han, H.-r.Guo

Isospin dependent nucleon-nucleus optical potential with Skyrme interactions

NUCLEAR REACTIONS 27Al, 56Fe, 208Pb(n, n'), (n, X), (p, p'), E<100 MeV; calculated σ. 27Al(n, n), E=1.5-96.0 MeV; 27Al(p, p), E=2.004-95.7 MeV; 56Fe(n, n), E=9.41-75.0 MeV; 56Fe(p, p), E=4.08-65.0 MeV; 208Pb(n, n), E=1.8-65.0 MeV; 208Pb(p, p), E=16.0-80 MeV; calculated σ(θ). 56Fe(n, X), (p, X), E=10-90 MeV; calculated radial dependence of neutron and proton microscopic optical potential (MOP). 27Al, 56Fe, 90Zr, 127I, 169Tm, 208Pb(p, X), E<120; calculated isospin effect values. Isospin dependent nucleon-nucleus optical potential calculations with Skyrme interactions. Comparison with experimental data.

doi: 10.1103/PhysRevC.80.024604
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2002LI17      Chin.Phys.Lett. 19, 306 (2002)

Z.-H.Li, W.-P.Liu, X.-X.Bai, Y.-B.Wang, G.Lian, Z.-C.Li, Q.-B.Shen, C.-J.Lin, S.Zeng, C.-B.Fu

Search for the Halo Effect in the 1H(6He, 6Li)n Reaction

NUCLEAR REACTIONS 1H(6He, 6Li), E=4.17 MeV/nucleon; measured σ(E, θ). 6He, 6Li deduced halo structure. DWBA analysis.

doi: 10.1088/0256-307X/19/3/306
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2002SH14      Nucl.Sci.Eng. 141, 78 (2002)

Q.-B.Shen

A Program for Automatically Searching Optimal Optical Potential Parameters in E ≤ 300 MeV Energy Region

NUCLEAR REACTIONS 208Pb(p, p), E=16-182 MeV; 56Fe(p, p), (p, X), E=4-156 MeV; 56Fe(n, n), (n, X), E=3.4-65 MeV; analyzed σ, σ(θ); deduced optical model parameters.

doi: 10.13182/NSE01-19CCA
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1995HA50      Chin.J.Nucl.Phys. 17, No 2, 129 (1995)

Y.-L.Han, Q.-B.Shen, Y.-Z.Zhuo

Properties of Hot Nuclear and Neutron Matter in a Relativistic Hartree-Fock Theory


1995SH44      Chin.J.Nucl.Phys. 17, No 1, 52 (1995)

Q.-B.Shen, J.-S.Zhang

A Quasiquantum Model for Calculating Multistep Direct Reactions of Continuum and Discrete Levels

NUCLEAR REACTIONS 11B(p, n), E ≈ 1-25 MeV; calculated σ(E), σ(θ) at some energies. Quasiquantum multi-step direct, DWBA theory.


1995SH45      Chin.J.Nucl.Phys. 17, No 1, 60 (1995)

Q.-B.Shen, J.-S.Zhang, Y.-L.Han, X.-X.Bai

Analyses of p-11B, p-11C and d-11C Reactions

NUCLEAR REACTIONS 9Be, 11B(p, X), E ≤ 40 MeV; calculated reaction σ(E), production σ(E) for many channels for 11B target. 1H(11B, 11C), E=66.12-89.58 MeV; calculated σ(θ). 11C(p, X), (d, X), E=1-25 MeV; calculated reaction σ(E) for many channels. Quasicontinuum multi-step direct, Hauser-Feshbach theories.


1994HA04      Nucl.Phys. A569, 732 (1994)

Y.-L.Han, Q.-B.Shen, Y.-Z.Zhuo, T.-M.Geng

Temperature-Dependent Relativistic Microscopic Optical Potential and the Mean Free Path of a Nucleon Based on Walecka's Model

doi: 10.1016/0375-9474(94)90382-4
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1994SH44      Chin.J.Nucl.Phys. 16, No 3, 243 (1994)

Q.-B.Shen, J.-S.Zhang

The Effect of Anisotropic Intranuclear Scattering on Angular Distribution of Nucleons in Preequilibrium Reaction

NUCLEAR REACTIONS 1H(n, n), E=50, 130 MeV; analyzed σ(θ); deduced model parameters; 93Nb(n, n'), E=14.6 MeV; 120Sn(p, p'), E=62 MeV; analyzed σ(θ, E(nucleon)). Preequilibrium reaction, anisotropic intranuclear scattering effect.


1992HA30      Phys.Rev. C46, 2396 (1992)

Y.-L.Han, Q.-B.Shen, Y.-Z.Zhuo

Temperature-Dependent Relativistic Microscopic Optical Potential of a Nucleon

NUCLEAR REACTIONS 208Pb(p, p), E=relativistic; calculated optical, Schrodinger-equivalent potentials, nucleon mean free paths. Walecka meson-nucleon model, thermofield dynamics models.

doi: 10.1103/PhysRevC.46.2396
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1991LI29      Nucl.Phys. A534, 48 (1991)

K.-F.Liu, H.-D.Luo, Z.Ma, M.Feng, Q.-B.Shen

Sum Rules for Nuclear Excitations with the Skyrme-Landau Interaction

NUCLEAR STRUCTURE 16O, 40,48Ca, 90Zr, 208Pb; calculated electric multipole, M1 excitation energy-weighted sum rules. Skyrme-Landau interactions.

doi: 10.1016/0375-9474(91)90557-M
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1991SH08      Phys.Rev. C43, 2773 (1991)

Q.-B.Shen, D.-C.Feng, Y.-Z.Zhuo

Neutron Relativistic Phenomenological and Microscopic Optical Potential

NUCLEAR REACTIONS 12C, 16O, 27Al, 56Fe, 63Cu, 107Ag, 181Ta, 208Pb, 209Bi, 238U(n, n), E=0.02-1 GeV; analyzed σ, other data. Phenomenological, microscopic optical potentials.

doi: 10.1103/PhysRevC.43.2773
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