NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = A.Csoto Found 34 matches. 2003OB04 Nucl.Phys. A719, 283c (2003) H.Oberhummer, A.Csoto, M.Fairbairn, H.Schlattl, M.M.Sharma Temporal variation of coupling constants and nucleosynthesis
doi: 10.1016/S0375-9474(03)00933-3
2001CS03 Nucl.Phys. A688, 511c (2001) Microscopic Calculations for Solar Nuclear Reactions NUCLEAR REACTIONS 4He(3He, γ), E=low; calculated S-factor and its correlations with quadrupole moment of 7Be and 7Li. 3He(3He, 2p), E=low; calculated resonances that may increase σ, none found. 7Be(p, γ), E=low calculated S-factor and its correlations with nuclear structure properties of 7Be and 8B.
doi: 10.1016/S0375-9474(01)00772-2
2001CS04 Nucl.Phys. A688, 560c (2001) A.Csoto, H.Oberhummer, H.Schlattl Fine-Tuning the Basic Forces of Nature Through the Triple-Alpha Process in Red Giant Stars NUCLEAR STRUCTURE 12C; calculated 2nd 0+ resonance energy for different sets of nuclear potentials. Cluster model. NUCLEAR REACTIONS 8Be(α, γ), E=low; calculated reaction rate as function of 2nd 0+ resonance energy in 12C; deduced 12C abundance following network calculations.
doi: 10.1016/S0375-9474(01)00787-4
2001OB02 Nucl.Phys. A689, 269c (2001) H.Oberhummer, A.Csoto, H.Schlattl Bridging the Mass Gaps at A = 5 and A = 8 in Nucleosynthesis
doi: 10.1016/S0375-9474(01)00841-7
2000CS01 Phys.Rev. C61, 024311 (2000) Low-Lying Continuum Structure in 8B and 8Li in a Microscopic Model NUCLEAR STRUCTURE 8B, 8Li; calculated resonances energies, widths. Analytic continuation of scattering matrix to complex energies.
doi: 10.1103/PhysRevC.61.024311
2000CS03 Phys.Rev. C61, 037601 (2000) Role of Spectroscopic Factors in the Potential-Model Description of the 7Be(p, γ)8B Reaction NUCLEAR REACTIONS 7Be(p, γ), E not given; calculated potential; deduced role of spectroscopic factors.
doi: 10.1103/PhysRevC.61.037601
2000CS06 Few-Body Systems 29, 121 (2000) Study of the 3He(4He, γ)7Be and 3H(4He, γ)7Li Reactions in an Extended Two-Cluster Model NUCLEAR REACTIONS 3H, 3He(α, γ), E(cm) < 5 MeV; calculated phase shifts, σ, astrophysical S-factors; deduced contribution from 6Li-plus-nucleon channel, related reaction mechanism features. Extended two-cluster model.
2000CS08 Acta Phys.Hung.N.S. 12, 149 (2000) A.Csoto, H.Oberhummer, H.Schlattl At the Edge of Nuclear Stability: Nonlinear quantum amplifiers
1999CS01 Nucl.Phys. A646, 387 (1999) Large-Space Cluster Model Calculations for the 3He(3He, 2p)4He and 3H(3H, 2n)4He Reactions NUCLEAR REACTIONS 3He(3He, 2p), 3H(t, 2n), E(cm) < 400 keV; calculated astrophysical S-factors; deduced no low-energy resonances. Microscopic cluster model. Comparison with data.
doi: 10.1016/S0375-9474(98)00638-1
1999CS02 Phys.Rev. C59, 1207 (1999); Erratum Phys.Rev. C62, 049901 (2000) Search for Excited States in 3H and 3He NUCLEAR STRUCTURE 3H, 3He; calculated d+N scattering matrices; deduced virtual excited states. Phenomenological interactions.
doi: 10.1103/PhysRevC.59.1207
1998CS02 Nucl.Phys. A631, 783c (1998) S-Matrix Studies of Resonances in A = 3, 4, 5, 6 and 12 Nucleon Systems
doi: 10.1016/S0375-9474(98)00109-2
1998CS03 Nucl.Phys. A636, 240 (1998) Effects of 8B Size on the Low-Energy 7Be(p, γ)8B Cross Section NUCLEAR REACTIONS 7Be(p, γ), E not given; calculated astrophysical S-factor; deduced dependence on 8B radius. Three-cluster model.
doi: 10.1016/S0375-9474(98)00200-0
1998HU18 Nucl.Phys. A638, 714 (1998) J.Humblet, A.Csoto, K.Langanke R-Matrix and K-Matrix Analysis of Elastic α-α Scattering NUCLEAR REACTIONS 4He(α, α), E(cm) < 40 MeV; analyzed phase shifts; deduced R-matrix, K-matrix parameters.
doi: 10.1016/S0375-9474(98)00419-9
1997CS01 Phys.Rev. C55, 536 (1997) S-Matrix and R-Matrix Determination of the Low-Energy 5He and 5Li Resonance Parameters NUCLEAR REACTIONS 4He(n, n), (p, p), E(cm) ≤ 15 MeV; analyzed phase shifts vs E. 5He, 5Li deduced resonance parameters. Microscopic cluster model.
doi: 10.1103/PhysRevC.55.536
1997CS02 Phys.Lett. 394B, 247 (1997) Off-Shell Effects in the Energy Dependence of the 7Be(p, γ)8B Astrophysical S Factor NUCLEAR REACTIONS, ICPND 7Be(p, γ), E(cm) ≤ 2.5 MeV; calculated astrophysical S-factor vs E; deduced off-shell effects role.
doi: 10.1016/S0370-2693(97)00031-2
1997CS03 Phys.Rev. C55, 2366 (1997) Nature of the First Excited State of 4He NUCLEAR REACTIONS 3H(p, p), E(cm) ≤ 1.5 MeV; analyzed σ(θ). 4He deduced level energy, width. Extended R-matrix method, cluster model, A=3 system distortions.
doi: 10.1103/PhysRevC.55.2366
1997CS05 Phys.Rev. C56, 631 (1997) A.Csoto, B.F.Gibson, G.L.Payne Parity Conserving γ Asymmetry in n-p Radiative Capture NUCLEAR REACTIONS 1H(polarized n, γ), E=cold; calculated parity conserving γ asymmetry; deduced weak pion coupling constant extraction related features.
doi: 10.1103/PhysRevC.56.631
1997CS07 Acta Phys.Hung.N.S. 6, 103 (1997) 7Be(p, γ)8B and the High-Energy Solar Neutrino Flux NUCLEAR REACTIONS 7Be(p, γ), E < 2.5 MeV; calculated astrophysical S-factors. Comparison with data.
1997PI07 Nucl.Phys. A618, 55 (1997) R.Pichler, H.Oberhummer, A.Csoto, S.A.Moszkowski Three-Alpha Structure in 12C NUCLEAR STRUCTURE 12C; calculated three-body resonances, Γ. Microscopic cluster model, complex scaling method.
doi: 10.1016/S0375-9474(97)00057-2
1996BR04 Nucl.Phys. A597, 66 (1996) Coulomb Displacement Energy and the Low-Energy Astrophysical S17 Factor for the 7Be(p, γ)8B Reaction NUCLEAR REACTIONS, ICPND 7Be(p, γ), E=low; calculated astrophysical S-factor. Shell model, solar neutrinos. NUCLEAR STRUCTURE 8B; calculated quadrupole moment. Shell model.
doi: 10.1016/0375-9474(95)00417-3
1996CS01 Phys.Rev. C53, 1444 (1996) Comment on ' Large-Space Shell-Model Calculations for Light Nuclei ' NUCLEAR STRUCTURE 7Li; calculated quadrupole moment vs α+t separation energy; deduced sensitivity, implications for 6Li, 5He nuclei studies. No-core, large space shell model.
doi: 10.1103/PhysRevC.53.1444
1996CS02 Phys.Rev. C53, 1589 (1996) A.Csoto, H.Oberhummer, R.Pichler Searching for Three-Nucleon Resonances NUCLEAR STRUCTURE 3n; calculated phase shifts; deduced resonances, J, π. 3H deduced possible excited state.
doi: 10.1103/PhysRevC.53.1589
1996CS03 Nucl.Phys. A601, 131 (1996) Parity-Violating α-Decay of the 3.56 MeV J(π), T = 0+, 1 State of 6Li NUCLEAR STRUCTURE 6Li; calculated level parity-violating α-decay width. Microscopic three-cluster model.
doi: 10.1016/0375-9474(96)00025-5
1996CS05 Nucl.Phys. A607, 62 (1996); Erratum Nucl.Phys. A609, 601 (1996) Low-Energy M1 Strength in the 7Li(p, γ0)8Be Reaction NUCLEAR REACTIONS, ICPND 7Li(p, γ), E(cm) ≤ 1.1 MeV; calculated astrophysical S-factor vs E. 8Be levels deduced spectroscopic amplitudes, M1 strength distribution. Microscopic cluster model.
doi: 10.1016/S0375-9474(96)00229-1
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
1995CS03 Phys.Rev. C52, 2809 (1995) Reply to ' Comment on ' Three-Body Resonances in 6He, 6Li, and 6Be, and the Soft Dipole Mode Problem of Neutron Halo Nuclei ' ' NUCLEAR STRUCTURE 12C, 11Li, 6He; analyzed resonancelike structure, decay features; deduced predicted low-lying dipole structure experimental check possibility in 6He, 11Li.
doi: 10.1103/PhysRevC.52.2809
1994CO10 Phys.Rev. C50, 1308 (1994) S.G.Cooper, R.S.Mackintosh, A.Csoto, R.G.Lovas Local 4He-p Potentials from Resonating-Group Method Phase Shifts NUCLEAR REACTIONS 4He(p, p), E ≤ 20 MeV; calculated phase shifts vs E; deduced phase equivalent potentials, local potentials comparison. Multi-channel resonating group method.
doi: 10.1103/PhysRevC.50.1308
1994CS01 Phys.Rev. C49, 818 (1994) Microscopic Description of the Beta Delayed Deuteron Emission from 6He RADIOACTIVITY 6He(β-); calculated β-decay transition probability, β-delayed deuteron spectra; deduced neutron halo role in α+d channel β-decay quenching. Dynamical cluster model. NUCLEAR REACTIONS 4He(d, d), E(cm) ≤ 5 MeV; calculated phase shifts vs E.
doi: 10.1103/PhysRevC.49.818
1994CS03 Phys.Rev. C49, 2244 (1994) Three-Body Resonances by Complex Scaling
doi: 10.1103/PhysRevC.49.2244
1994CS04 Phys.Rev. C49, 3035 (1994) Three-Body Resonances in 6He, 6Li, and 6Be, and the Soft Dipole Mode Problem of Neutron Halo Nuclei NUCLEAR STRUCTURE 6He, 6Li, 6Be; calculated levels, Γ. 6He deduced no soft dipole mode evidence. Complex scaling method, microscopic three-cluster model.
doi: 10.1103/PhysRevC.49.3035
1993CS02 Phys.Rev.Lett. 70, 1389 (1993) A.Csoto, R.G.Lovas, A.T.Kruppa Two-Pole Structure of the (3/2)+ Resonance of 5He in a Dynamical Microscopic Model NUCLEAR REACTIONS 3H(d, d), E ≤ 150 keV; 4He(n, n), ≤ 6 MeV; analyzed phase shifts. 5He, 5Li deduced 3/2 resonance characteristics. Dynamical microscopic model.
doi: 10.1103/PhysRevLett.70.1389
1993CS04 Phys.Rev. C48, 165 (1993) Neutron Halo of 6He in a Microscopic Model NUCLEAR STRUCTURE 6He, 6Li, 6Be; calculated levels, (L, S) components weights. 6He deduced neutron halo evidence, two-neutron separation energy, nucleon rms radii. Microscopic model.
doi: 10.1103/PhysRevC.48.165
1993CS06 Phys.Lett. 315B, 24 (1993) Proton Skin of 8B in a Microscopic Model NUCLEAR STRUCTURE 8B, 8Li; calculated quadrupole moment, point nucleon rms radii; deduced nucleon skin thickness. Dynamical microscopic cluster model.
doi: 10.1016/0370-2693(93)90152-8
1992CS04 Phys.Rev. C46, 576 (1992) Dynamical Microscopic Three-Cluster Description of 6Li NUCLEAR STRUCTURE 6Li; calculated d+α, α+p+n breakup spectroscopic factors, ground state energy vs clusterization components. Dynamical microscopic cluster model.
doi: 10.1103/PhysRevC.46.576
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