NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = M.H.Mahzoon Found 7 matches. 2020AT01 Phys.Rev. C 101, 044303 (2020) M.C.Atkinson, M.H.Mahzoon, M.A.Keim, B.A.Bordelon, C.D.Pruitt, R.J.Charity, W.H.Dickhoff Dispersive optical model analysis of 208Pb generating a neutron-skin prediction beyond the mean field NUCLEAR REACTIONS 208Pb(p, X), (n, X), (p, p), (n, n), E=10-200 MeV; 208Pb(e, e), E=502 MeV; calculated reaction σ(E), differential σ(E, θ), analyzing powers Ay(θ) using dispersive optical model (DOM). Comparison with experimental data. NUCLEAR STRUCTURE 208Pb; calculated neutron and proton single-particle energy levels, charge density, orbital occupation and depletion numbers, spectroscopic factors, binding energies, momentum distributions of protons and neutrons. 40,48Ca, 208Pb; calculated proton and neutron point distributions, and neutron skins. Hartree-Fock and dispersive optical model (DOM) calculations. Comparison with experimental data. Relevance to nuclear equation of state.
doi: 10.1103/PhysRevC.101.044303
2017DI03 J.Phys.(London) G44, 033001 (2017) W.H.Dickhoff, R.J.Charity, M.H.Mahzoon Novel applications of the dispersive optical model
doi: 10.1088/1361-6471/44/3/033001
2017MA76 Phys.Rev.Lett. 119, 222503 (2017) M.H.Mahzoon, M.C.Atkinson, R.J.Charity, W.H.Dickhoff Neutron Skin Thickness of 48Ca from a Nonlocal Dispersive Optical-Model Analysis NUCLEAR REACTIONS 48Ca(n, n), E not given; analyzed available data; deduced σ, σ(θ), neutron and proton numbers, and the charge distributions.
doi: 10.1103/PhysRevLett.119.222503
2015RO17 Phys.Rev. C 92, 044607 (2015) A.Ross, L.J.Titus, F.M.Nunes, M.H.Mahzoon, W.H.Dickhoff, R.J.Charity Effects of nonlocal potentials on (p, d) transfer reactions NUCLEAR REACTIONS 40Ca(p, d)39Ca, E=20, 35, 50 MeV; 40Ca(p, p), E=50 MeV; calculated σ(θ) distributions using nonlocal potential obtained from non-local dispersive optical model (DOM) and DOM-phase equivalent (PE), combined with DWBA. Comparison with Perey-Buck (PB) optical potential predictions, and with experimental data.
doi: 10.1103/PhysRevC.92.044607
2014DU15 Phys.Rev. C 90, 061603 (2014) H.Dussan, M.H.Mahzoon, R.J.Charity, W.H.Dickhoff, A.Polls Elastic nucleon-nucleus scattering as a direct probe of correlations beyond the independent-particle model NUCLEAR REACTIONS 40Ca(p, p), (n, n), E<200 MeV; analyzed scattering and structure data using the full nonlocal treatment of the dispersive optical model (DOM). Discussed application for inverse kinematics reactions.
doi: 10.1103/PhysRevC.90.061603
2014MA18 Phys.Rev.Lett. 112, 162503 (2014) M.H.Mahzoon, R.J.Charity, W.H.Dickhoff, H.Dussan, S.J.Waldecker Forging the Link between Nuclear Reactions and Nuclear Structure NUCLEAR REACTIONS 40Ca(n, n), (p, p), E<200 MeV; calculated σ, σ(θ), spectral strength. Comparison with experimental data.
doi: 10.1103/PhysRevLett.112.162503
2013SO11 Phys.Rev. C 87, 054329 (2013) L.G.Sobotka, W.W.Buhro, R.J.Charity, J.M.Elson, M.F.Jager, J.Manfredi, M.H.Mahzoon, A.M.Mukhamedzhanov, V.Eremenko, M.McCleskey, R.G.Pizzone, B.T.Roeder, A.Spiridon, E.Simmons, L.Trache, M.Kurokawa, P.Navratil Proton decay of excited states in 12N and 13O and the astrophysical 11C(p, γ)12N reaction rate NUCLEAR REACTIONS 9Be(13O, X), E=30.3 MeV/nucleon, [13O secondary beam from 1H(14N, X), E=38 MeV/nucleon primary reaction]; measured particle spectra, E(p), I(p), widths using MARS spectrometer at Texas AM cyclotron facility. Invariant mass method. R-matrix analysis. 11C, 12N, 13O; deduced levels, J, π, one-proton and two-proton decay branching ratios. 11C(p, γ)12N; deduced astrophysical reaction rates and S(E) factors.
doi: 10.1103/PhysRevC.87.054329
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