NSR Query Results
Output year order : Descending NSR database version of May 1, 2024. Search: Author = M.Ueda Found 28 matches. 2021CA10 Eur.Phys.J. A 57, 11 (2021) Semi-classical approaches to heavy-ion reactions: fusion, rainbow, and glory NUCLEAR REACTIONS 208Pb(11Li, X), 209Bi(6Li, X), (7Li, X), E(cm)=10-40 MeV; analyzed available data; deduced fusion σ.
doi: 10.1140/epja/s10050-020-00312-8
2011NA01 C.R.Physique 12, 13 (2011) The Efimov effect in lithium 6 ATOMIC PHYSICS 6Li; analyzed experimental data, scattering lengths as a function of magnetic field, recombination coefficients; deduced consistency with the Efimov effect.
doi: 10.1016/j.crhy.2010.12.002
2007IT05 Nucl.Phys. A787, 267c (2007) M.Ito, K.Yabana, T.Nakatsukasa, M.Ueda Fusion reaction of halo nuclei : A real-time wave-packet method for three-body tunneling dynamics NUCLEAR REACTIONS 209Bi(10Be, X), (11Be, X), E(cm)=36-50 MeV; 238U(α, X), (6He, X), E(cm)=14-32 MeV; calculated fusion σ. Three-body model, time-dependent wave-packet method to solve Schroedinger equation. Comparison with data.
doi: 10.1016/j.nuclphysa.2006.12.042
2007SA43 Nucl.Phys. A790, 737c (2007) Symmetry breaking in scalar, spinor, and rotating Bose-Einstein condensates
doi: 10.1016/j.nuclphysa.2007.03.122
2006IT04 Phys.Lett. B 637, 53 (2006) M.Ito, K.Yabana, T.Nakatsukasa, M.Ueda Suppressed fusion cross section for neutron halo nuclei NUCLEAR REACTIONS 209Bi(10B, X), (11B, X), E(cm)=30-50 MeV; 238U(α, X), (6He, X), E(cm)=14-32 MeV; calculated fusion σ. Three-body time-dependent wave-packet model, comparison with data.
doi: 10.1016/j.physletb.2006.03.027
2004HU06 Nucl.Phys. A734, 445 (2004) M.S.Hussein, A.J.Sargeant, M.P.Pato, M.Ueda Variance of the decay intensity of superdeformed bands
doi: 10.1016/j.nuclphysa.2004.01.082
2004HU10 Nucl.Phys. A734, E61 (2004) M.S.Hussein, M.Ueda, A.J.Sargeant, M.P.Pato Resonances and the thermonuclear reaction rate NUCLEAR REACTIONS 12C(n, γ), E=low; calculated astrophysical reaction rate, resonance effects.
doi: 10.1016/j.nuclphysa.2004.03.020
2004HU14 Prog.Theor.Phys.(Kyoto), Suppl. 154, 146 (2004) M.S.Hussein, A.J.Sargeant, M.P.Pato, N.Takigawa, M.Ueda Energy Averages over Regular and Chaotic States in the Decay Out of Superdeformed Bands
doi: 10.1143/PTPS.154.146
2004NA27 Prog.Theor.Phys.(Kyoto), Suppl. 154, 85 (2004) T.Nakatsukasa, K.Yabana, M.Ito, M.Kobayashi, M.Ueda Fusion Reaction of Halo Nuclei: Proton Halo versus Neutron Halo
doi: 10.1143/PTPS.154.85
2004SA30 Phys.Rev. C 69, 067301 (2004) A.J.Sargeant, M.S.Hussein, M.P.Pato, N.Takigawa, M.Ueda Addendum: Attenuation of the intensity within a superdeformed band
doi: 10.1103/PhysRevC.69.067301
2004UE04 Nucl.Phys. A738, 288 (2004) M.Ueda, K.Yabana, T.Nakatsukasa Absorbing Boundary Condition Approach to Breakup Reactions of One-Neutron Halo Nuclei NUCLEAR REACTIONS 12C(11Be, n10Be), E=50, 67 MeV/nucleon; calculated fragments relative energy, σ(θ). Absorbing boundary condition method, comparison with data.
doi: 10.1016/j.nuclphysa.2004.04.047
2004UE05 Phys.Rev. C 70, 025802 (2004) M.Ueda, A.J.Sargeant, M.P.Pato, M.S.Hussein Resonances and thermonuclear reaction rates for charged particle collisions NUCLEAR REACTIONS 12C(p, γ), E=low; calculated astrophysical reaction rate, resonance contribution. Analytic expression.
doi: 10.1103/PhysRevC.70.025802
2004YA19 Nucl.Phys. A738, 303 (2004) K.Yabana, M.Ito, M.Kobayashi, M.Ueda, T.Nakatsukasa Fusion reaction of halo nuclei: a time-dependent approach
doi: 10.1016/j.nuclphysa.2004.04.050
2003UE01 Phys.Rev. C 67, 014606 (2003) M.Ueda, K.Yabana, T.Nakatsukasa Application of an absorbing boundary condition to nuclear breakup reactions NUCLEAR REACTIONS 12C(16O, 16O), E=139.2 MeV; calculated elastic scattering matrix elements. 58Ni(d, np), E=80 MeV; calculated deuteron breakup matrix elements. Absorbing boundary condition method, comparison with coupled discretized continuum channels approach.
doi: 10.1103/PhysRevC.67.014606
2003YA17 Nucl.Phys. A722, 261c (2003) K.Yabana, M.Ueda, T.Nakatsukasa Time-dependent wave-packet approach for fusion reactions of halo nuclei NUCLEAR REACTIONS 208Pb(11Be, X), E=30-45 MeV; calculated wave-packet dynamics, fusion probability.
doi: 10.1016/S0375-9474(03)01375-7
2002SA04 Phys.Rev. C65, 024302 (2002); Comment Phys.Rev. C 68, 069801 (2003) A.J.Sargeant, M.S.Hussein, M.P.Pato, N.Takigawa, M.Ueda Attenuation of the Intensity within a Superdeformed Band
doi: 10.1103/PhysRevC.65.024302
2002SA26 Nucl.Phys. A705, 119 (2002) K.Saito, M.Ueda, K.Tsushima, A.W.Thomas Structure Functions of Unstable Lithium Isotopes NUCLEAR STRUCTURE 6,7,8,9,11Li; calculated neutron and proton separation energies, radii, single-particle level energies, spin-average and spin-dependent structure functions. Comparisons with data.
doi: 10.1016/S0375-9474(02)00624-3
2002SA52 Phys.Rev. C 66, 064301 (2002) A.J.Sargeant, M.S.Hussein, M.P.Pato, M.Ueda Energy averages and fluctuations in the decay out of superdeformed bands
doi: 10.1103/PhysRevC.66.064301
2002UE04 Prog.Theor.Phys.(Kyoto), Suppl. 146, 634 (2002) M.Ueda, A.J.Sargeant, M.P.Pato, M.S.Hussein Evaluation of Effective Astrophysical S Factor for Non-Resonant Reactions
doi: 10.1143/PTPS.146.634
2002YA19 Prog.Theor.Phys.(Kyoto), Suppl. 146, 329 (2002) K.Yabana, M.Ueda, T.Nakatsukasa Absorbing Boundary Condition Approach for Breakup Reactions of Halo Nuclei NUCLEAR REACTIONS 58Ni(d, d), E=80 MeV; calculated σ(θ). 12C(n, n), E=5-100 MeV; calculated σ. 12C(11Be, X), E=5-100 MeV/nucleon; calculated elastic breakup σ. Absorbing boundary condition approach, comparison with Eikonal approximation.
doi: 10.1143/PTPS.146.329
2000SA01 Phys.Rev. C61, 011302 (2000) A.J.Sargeant, M.S.Hussein, M.P.Pato, M.Ueda Saturation of the Width of the Strength Function
doi: 10.1103/PhysRevC.61.011302
2000UE01 Phys.Rev. C61, 045801 (2000) M.Ueda, A.J.Sargeant, M.P.Pato, M.S.Hussein Effective Astrophysical S Factor for Nonresonant Reactions NUCLEAR REACTIONS 7Be(p, γ), E not given; calculated effective astrophysical S factors. Asymptotic expansion.
doi: 10.1103/PhysRevC.61.045801
1999UE02 Nucl.Phys. A648, 229 (1999) M.Ueda, M.P.Pato, M.S.Hussein, N.Takigawa Glory ' In the Shadow of the Rainbow ' NUCLEAR REACTIONS 90Zr(α, α), E=40-200 MeV; calculated σ(θ), forward scattering features; deduced rainbow scattering shadow effect. Semiclassical interpretation. Sum-of-differences approach.
doi: 10.1016/S0375-9474(99)00021-4
1998UE02 Phys.Rev.Lett. 81, 1809 (1998) Forward Glory Phenomenon in the Dark-Side of Heavy-Ion Nuclear Rainbow Scattering NUCLEAR REACTIONS 90Zr(α, α), E=40 MeV; calculated scattering amplitude vs θ; deduced rainbow scattering components, absorption role. Comparison of quantum, semiclassical approaches.
doi: 10.1103/PhysRevLett.81.1809
1996UE01 Nucl.Phys. A598, 273 (1996) Forward Nuclear Glory Scattering of a Halo Nucleus NUCLEAR REACTIONS 12C(11Li, 11Li), (11C, 11C), E ≈ 60 MeV/nucleon; 28Si(7Li, 7Li), E=178 MeV; 28Si(11Li, 11Li), E=319 MeV; calculated sum-of-differences σ vs θ, forward angle scattering amplitude, deflection function. Forward nuclear glory.
doi: 10.1016/0375-9474(95)00481-5
1996UE07 Prog.Theor.Phys.(Kyoto), Suppl. 124, 135 (1996) Forward Nuclear Glory Scattering of a Halo Nucleus NUCLEAR REACTIONS 12C(11Li, 11Li), (11C, 11C), E not given; calculated forward-angle scatering amplitudes; deduced neutron halo role.
doi: 10.1143/PTPS.124.135
1992TA16 Phys.Lett. 288B, 244 (1992) N.Takigawa, M.Ueda, M.Kuratani, H.Sagawa Elastic Scattering of a Halo Nucleus at Medium Energies NUCLEAR REACTIONS 12C(11Li, 11Li), E=360 MeV; calculated σ(θ), with, without neutron halo; deduced breakup reaction role for halo nuclei scattering, Glauber theory optical limit approximation validity features.
doi: 10.1016/0370-2693(92)91098-T
1984TA19 J.Nucl.Sci.Technol.(Tokyo) 21, 577 (1984) A.Takahashi, J.Yamamoto, K.Oshima, M.Ueda, M.Fukazawa, Y.Yanagi, J.Miyaguchi, K.Sumita Measurements of Double Differential Neutron Emission Cross Sections for Fusion Reactor Candidate Elements NUCLEAR REACTIONS 2H, O, Si, 19F, Ti, 55Mn, 209Bi(n, n), E=0.3-14 MeV; Li, 9Be, Pb, 209Bi(n, n), E=0.5-14 MeV; measured σ(θn, En).
doi: 10.1080/18811248.1984.9731087
Back to query form |