NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = A.Adahchour Found 11 matches. 2017AD32 Phys.Rev. C 96, 054319 (2017) Three-body continuum of 26O NUCLEAR STRUCTURE 26O; calculated 24O+n+n three-body eigenphases for J=0+, 1- and 2+; deduced narrow resonance for J=2+ near 1.3 MeV with Γ ≈ 0.4 MeV, in agreement with recent experimental data. Hyperspherical formalism for 24O+n and n+n interactions, and R-matrix technique to derive wave functions and associated phase shifts.
doi: 10.1103/PhysRevC.96.054319
2010AD02 J.Phys.(London) G37, 045102 (2010) Three-body structure of 18Ne in a microscopic model NUCLEAR STRUCTURE 18Ne, 18O; analyzed spectroscopy of low-lying states; deduced the resonance width. Analytical Continuation in the Coupling Constant (ACCC).
doi: 10.1088/0954-3899/37/4/045102
2008AD16 Nucl.Phys. A813, 252 (2008) Microscopic cluster model of 5H and 5He (T = 3/2) NUCLEAR STRUCTURE 5H, 5He; calculated levels, cluster configurations. Microscopic three cluster model with hyperspherical formalism. Comparison with other models.
doi: 10.1016/j.nuclphysa.2008.09.008
2006AD22 Phys.Lett. B 639, 447 (2006) Core excitations in 8He and 7He NUCLEAR STRUCTURE 7,8He; calculated levels, cluster configurations. Microscopic three cluster model.
doi: 10.1016/j.physletb.2006.05.092
2005AD03 Eur.Phys.J. A 23, 435 (2005) A test of the zero-range DWBA method at astrophysical energies NUCLEAR REACTIONS 13C(α, n), E=0-5 MeV; calculated phase shifts, transition amplitudes. Comparison of DWBA and microscopic cluster model.
doi: 10.1140/epja/i2004-10113-x
2005CO07 Nucl.Phys. A752, 522c (2005) A.Coc, C.Angulo, E.Vangioni-Flam, P.Descouvemont, A.Adahchour Big Bang nucleosynthesis, microwave anisotropy, and the light element abundances
doi: 10.1016/j.nuclphysa.2005.02.057
2005DE46 Nucl.Phys. A758, 783c (2005) P.Descouvemont, A.Adahchour, C.Angulo, A.Coc, E.Vangioni-Flam Big-Bang reaction rates within the R-matrix model NUCLEAR REACTIONS 3He(d, p), E(cm) < 1 MeV; 7Li(p, α), E(cm)<10 MeV; 2H(p, γ), (d, n), (d, p), 3H(d, n), (α, γ), 3He(n, p), (α, γ), 7Be(n, p), E=low; analyzed astrophysical S-factors, reactions rates.
doi: 10.1016/j.nuclphysa.2005.05.140
2004DE48 At.Data Nucl.Data Tables 88, 203 (2004) P.Descouvemont, A.Adahchour, C.Angulo, A.Coc, E.Vangioni-Flam Compilation and R-matrix analysis of Big Bang nuclear reaction rates NUCLEAR REACTIONS 2H(p, γ), (d, n), (d, p), 3H(d, n), (α, γ), 3He(n, p), (d, p), (α, γ), 7Li(p, α), 7Be(n, p), E=low; analyzed σ; deduced astrophysical S-factors, reaction rates.
doi: 10.1016/j.adt.2004.08.001
2003AD05 J.Phys.(London) G29, 395 (2003) R-matrix analysis of the 3He(n, p)3H and 7Be(n, p)7Li reactions NUCLEAR REACTIONS 3He(n, p), E(cm) < 10 MeV; 7Be(n, p), E(cm) < 20 MeV; analyzed σ; deduced R-matrix parameters. 4He, 8Be levels deduced neutron and proton resonance widths. Astrophysical implications discussed.
doi: 10.1088/0954-3899/29/2/315
1995AD15 Phys.Lett. 356B, 445 (1995) A.Adahchour, D.Baye, P.Descouvemont 14Be in a Lagrange-Mesh Calculation NUCLEAR STRUCTURE 14Be; calculated binding energy, matter radius. Three-body approach, Lagrange-mesh technique, microscopic n-12Be potential.
doi: 10.1016/0370-2693(95)00860-N
1994AD08 Nucl.Phys. A579, 305 (1994) A.Adahchour, D.Baye, P.Descouvemont Microscopic Derivation of Local Interactions between p-Shell Nuclei NUCLEAR REACTIONS 15N(12C, 12C), (16O, 16O), 13C(16O, 16O), E(cm) ≈ 15-65 MeV; calculated phase shifts vs E. Single-channel, two-center generator coordinate method.
doi: 10.1016/0375-9474(94)90808-7
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