NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = T.Shoppa Found 14 matches. 2000SH17 Phys.Rev. C61, 054902 (2000) T.D.Shoppa, S.E.Koonin, R.Seki Effect of the Source Charge on Charged-Boson Interferometry
doi: 10.1103/PhysRevC.61.054902
1998AD12 Rev.Mod.Phys. 70, 1265 (1998) E.G.Adelberger, S.M.Austin, J.B.Bahcall, A.B.Balantekin, G.Bogaert, L.S.Brown, L.Buchmann, F.E.Cecil, A.E.Champagne, L.de Braeckeleer, C.A.Duba, S.R.Elliott, S.J.Freedom, M.Gai, G.Goldring, C.R.Gould, A.Gruzinov, W.C.Haxton, K.M.Heeger, E.Henley, C.W.Johnson, M.Kamionkowski, R.W.Kavanagh, S.E.Koonin, K.Kubodera, K.Langanke, T.Motobayashi, V.Pandharipande, P.Parker, R.G.H.Robertson, C.Rolfs, R.F.Sawyer, N.Shaviv, T.D.Shoppa, K.A.Snover, E.Swanson, R.E.Tribble, S.Turck-Chieze, J.F.Wilkerson Solar Fusion Cross Sections NUCLEAR REACTIONS 7Be, 12,13C, 15N, 16,17,18O(p, γ), 14,15N, 17,18O(p, α), 7Li(d, p), 3He(p, e+), (α, γ), (3He, 2p), 1H(p, e+), E=low; compiled, analyzed S-factor data, calculations; deduced implications for solar neutrino flux calculations.
doi: 10.1103/RevModPhys.70.1265
1998CH05 Phys.Rev. C57, R475 (1998) J.C.Chow, A.C.Morton, R.E.Azuma, N.Bateman, R.N.Boyd, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, W.Galster, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, J.D.King, G.Roy, T.Shoppa, A.Shotter Three-Particle Breakup of the Isobaric Analog State in 17F RADIOACTIVITY 17Ne(β+) [from Mg, O(p, X)]; measured β-delayed pα(12C)-coin. 17F deduced IAS p, α branching ratios. Implications for stellar helium burning discussed.
doi: 10.1103/PhysRevC.57.R475
1998JE04 Phys.Rev. C58, 579 (1998) B.K.Jennings, S.Karataglidis, T.D.Shoppa Direct Capture Astrophysical S Factors at Low Energy NUCLEAR REACTIONS 16O(p, γ), E < 3 MeV; 7Be(p, γ), E < 0.4 MeV; calculated astrophysical S-factors; deduced low-energy behaviour mechanism.
doi: 10.1103/PhysRevC.58.579
1998JE11 Phys.Rev. C58, 3711 (1998) B.K.Jennings, S.Karataglidis, T.D.Shoppa Extrapolation of the Astrophysical S Factor for 7Be(p, γ)8B to Solar Energies NUCLEAR REACTIONS 7Be(p, γ), E < 3 MeV; calculated astrophysical S-factor; deduced high-energy extrapolation model dependence. Comparisons with data.
doi: 10.1103/PhysRevC.58.3711
1997CA03 Z.Phys. A356, 399 (1997) TDHF Study of the He+ Collision on Atomic He Targets at the 8Be Ground State Energy ATOMIC PHYSICS 4He(α, X), E(cm)=92.1 keV; calculated electron wave function, amount of charge included in sphere time evolution. Time dependent Hartree-Fock approach, 8Be resonance included.
doi: 10.1007/s002180050195
1996LA06 Phys.Lett. 369B, 211 (1996) K.Langanke, T.D.Shoppa, C.A.Barnes, C.Rolfs Energy Loss, Electron Screening and the Astrophysical 3He(d, p)4He Cross Section NUCLEAR REACTIONS, ICPND 3He(d, p), E=0-40 keV; analyzed data; deduced astrophysical S-factor vs E. Proton, deuteron beams energy loss in helium gas.
doi: 10.1016/0370-2693(96)00066-4
1996SE09 Phys.Lett. 383B, 133 (1996) R.Seki, T.D.Shoppa, A.Kohama, K.Yazaki Nuclear Correlation and Finite Interaction-Range Effects in High-Energy (e, e'p) Nuclear Transparency NUCLEAR STRUCTURE 16O, 40Ca; calculated nuclear transparency at proton momentum of 4.49 GeV/c in (e, e'p) reaction. Glauber multiple scattering, all orders included.
doi: 10.1016/0370-2693(96)00735-6
1996SH15 Nucl.Phys. A605, 387 (1996) T.D.Shoppa, M.Jeng, S.E.Koonin, K.Langanke, R.Seki Electron Screening in Molecular Fusion Reactions NUCLEAR REACTIONS, ICPND 2H(d, p), E ≤ 20 keV; 3H(d, n), E(cm) ≤ 30 keV; calculated astrophysical S-factor. Time-dependent Hartree-Fock, molecular fusion, electron screening, dynamical wave function evolution.
doi: 10.1016/0375-9474(96)00183-2
1995CS01 Phys.Rev. C52, 1130 (1995) A.Csoto, K.Langanke, S.E.Koonin, T.D.Shoppa 7Be(p, γ)8B Cross Section and the Properties of 7Be NUCLEAR REACTIONS, ICPND 7Be(p, γ), E(cm) ≤ 2.5 MeV; calculated astrophysical S-factor vs E. Three-cluster resonating group model.
doi: 10.1103/PhysRevC.52.1130
1995LA17 Phys.Rev. C52, 1709 (1995) Reply to ' Comment on ' E2 Contribution to the 8B → p + 7Be Coulomb Dissociation Cross Section ' ' NUCLEAR REACTIONS, ICPND 7Be(p, γ), E=low; analyzed Coulomb dissociation data analyses; deduced need for better data to determine astrophysical S-factor reliably.
doi: 10.1103/PhysRevC.52.1709
1994LA08 Phys.Rev. C49, R1771 (1994); Erratum Phys.Rev. C51, 2844 (1995) E2 Contribution to the 8B → p + 7Be Coulomb Dissociation Cross Section NUCLEAR REACTIONS 208Pb(8B, p7Be), E=46.5 MeV/nucleon; analyzed Coulomb dissociation σ; deduced E1, E2 contributions, 7Be(p, γ) astrophysical S-factor reduction at solar energies.
doi: 10.1103/PhysRevC.49.R1771
1993SH14 Phys.Rev. C48, 837 (1993) T.D.Shoppa, S.E.Koonin, K.Langanke, R.Seki One- and Two-Electron Atomic Screening in Fusion Reactions NUCLEAR REACTIONS 3He, 2H(d, d), E=low; calculated electron screening potential vs internuclear separation. Time-dependent Hartree-Fock, classical motion of nuclei.
doi: 10.1103/PhysRevC.48.837
1992SH11 Phys.Rev. C46, 382 (1992) Determining the 12C(α, γ)16O Cross Section from Coulomb Dissociation NUCLEAR REACTIONS Pb(16O, α12C), E=10-400 MeV/nucleon; calculated Coulomb dissociation σ(θ, Eγ); deduced multipole contributions, E2 dominance, relevance to 12C(α, γ) reaction σ.
doi: 10.1103/PhysRevC.46.382
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