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NSR database version of May 3, 2024.

Search: Author = V.S.Melezhik

Found 11 matches.

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2022VA01      Eur.Phys.J. A 58, 34 (2022)

D.Valiolda, D.Janseitov, V.Melezhik

Investigation of low-lying resonances in breakup of halo nuclei within the time-dependent approach

NUCLEAR REACTIONS ²⁰⁸Pb(¹¹Be, X), E=5-70 MeV/nucleon; analyzed available data; calculated σ(E), resonant states J, π within the non-perturbative semiclassical and quantum-quasiclassical time-dependent approaches.

doi: 10.1140/epja/s10050-022-00684-z
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2022VA12      Phys.Part. and Nucl.Lett. 19, 477 (2022)

D.S.Valiolda, D.M.Janseitov, V.S.Melezhik

Study of Nuclear Contribution to Breakup Cross Section of ¹¹Be Halo Nuclei within Time-Dependent Approach

NUCLEAR REACTIONS ²⁰⁸Pb(¹¹Be, n), E=5-30 MeV/nucleon; analyzed available data. ¹⁰Be; calculated σ, the influence of nuclear interaction to the Coulomb breakup of one-neutron halo nuclei on a heavy target has been studied within the non-perturbative time-dependent approach.

doi: 10.1134/S1547477122050442
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2003BA97      Nucl.Phys. A722, 328c (2003)

D.Baye, P.Capel, V.S.Melezhik

Time-dependent analysis of the Coulomb breakup of weakly-bound nuclei

doi: 10.1016/S0375-9474(03)01385-X
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2003CA01      Phys.Lett. 552B, 145 (2003)

P.Capel, D.Baye, V.S.Melezhik

Supersymmetric elimination of forbidden states in the Coulomb breakup of the ¹¹Be halo nucleus

NUCLEAR REACTIONS Pb(¹¹Be, ¹⁰Be), E=72 MeV/nucleon; calculated Coulomb breakup σ vs fragment relative energy. Time-dependent calculations, phase-equivalent potentials, comparison with data.

doi: 10.1016/S0370-2693(02)03128-3
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2003CA25      Phys.Rev. C 68, 014612 (2003)

P.Capel, D.Baye, V.S.Melezhik

Time-dependent analysis of the breakup of halo nuclei

NUCLEAR REACTIONS ²⁰⁸Pb(¹¹Be, n¹⁰Be), (¹⁵C, n¹⁴C), (¹¹Be, ¹¹Be'), (¹⁵C, ¹⁵C'), E ≈ 70 MeV/nucleon; calculated breakup and inelastic σ. Semiclassical time-dependent Schrodinger equation.

doi: 10.1103/PhysRevC.68.014612
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2002ME27      Prog.Theor.Phys.(Kyoto), Suppl. 146, 457 (2002)

V.S.Melezhik, D.Baye

Time-Dependent Analysis of the Coulomb Breakup Determination of the Astrophysical S Factor

NUCLEAR REACTIONS ²⁰⁸Pb(¹⁷F, p¹⁶O), E not given; analyzed Coulomb breakup data. ¹⁶O(p, γ), E=0-2 MeV; deduced astrophysical S-factor.

doi: 10.1143/PTPS.146.457
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2001ME18      Nucl.Phys. A689, 563c (2001)

V.S.Melezhik, D.Baye

Time-Dependent Approach to Breakup of Nuclei with Neutron and Proton Halo

NUCLEAR REACTIONS ²⁰⁸Pb(¹¹Be, n¹⁰Be), (¹⁷F, p¹⁶O), E=0-6 MeV; calculated breakup σ.

doi: 10.1016/S0375-9474(01)00905-8
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2001ME25      Phys.Rev. C64, 054612 (2001)

V.S.Melezhik, D.Baye

Time-Dependent Analysis of the Coulomb Breakup Method for Determining the Astrophysical S Factor

NUCLEAR REACTIONS ²⁰⁸Pb(¹⁷F, p¹⁶O), E ≈ 10-72 MeV/nucleon; calculated breakup σ, σ vs fragments relative energy. ¹⁶O(p, γ), E(cm) ≈ 0.3-2 MeV; calculated astrophysical S-factor. Time-dependent mesh method.

doi: 10.1103/PhysRevC.64.054612
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1999ME12      Phys.Rev. C59, 3232 (1999)

V.S.Melezhik, D.Baye

Nonperturbative Time-Dependent Approach to Breakup of Halo Nuclei

NUCLEAR REACTIONS ²⁰⁸Pb(¹¹Be, n¹⁰Be), E=72 MeV/nucleon; calculated σ(E). Nonperturbative time-dependent approach.

doi: 10.1103/PhysRevC.59.3232
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1990BR12      Nucl.Phys. A513, 316 (1990)

L.Bracci, G.Fiorentini, V.S.Melezhik, G.Mezzorani, P.Quarati

Atomic Effects in the Determination of Nuclear Cross Sections of Astrophysical Interest

NUCLEAR STRUCTURE ⁷Li, ⁷Be, ¹¹B, ¹²C, ¹⁴N, ¹⁶O; calculated proton induced reaction atomic correction factor.

ATOMIC PHYSICS ⁷Li, ⁷Be, ¹¹B, ¹²C, ¹⁴N, ¹⁶O; calculated proton induced reaction atomic correction factor.

doi: 10.1016/0375-9474(90)90101-Q
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1989BO58      Yad.Fiz. 50, 1365 (1989); Sov.J.Nucl.Phys. 50, 848 (1989)

L.N.Bogdanova, V.E.Markushin, V.S.Melezhik, L.I.Ponomarev

Effect of the Nuclear Interaction in the Muonic Molecule dtμ on the Probability for the Muon Sticking to Helium in the Reaction dtμ → μα + n

Note: The following list of authors and aliases matches the search parameter V.S.Melezhik: , V.S.MELEZHIK