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NSR database version of May 6, 2024.

Search: Author = D.M.Zazulin

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2022DU11      Nucl.Phys. A1028, 122543 (2022)

S.B.Dubovichenko, N.A.Burkova, D.M.Zazulin

Reaction rate of radiative p¹²N capture

NUCLEAR REACTIONS ¹²N(p, γ), E(cm)<10 MeV; calculated S factors, reaction rates using modified potential cluster models (MPCM).Comparison with available data.

doi: 10.1016/j.nuclphysa.2022.122543
Citations: PlumX Metrics

2019DU16      Nucl.Phys. A987, 46 (2019)

S.B.Dubovichenko, N.A.Burkova, A.V.Dzhazairov-Kakhramanov, R.Ya.Kezerashvili, Ch.T.Omarov, A.S.Tkachenko, D.M.Zazulin

Radiative ³He(²H, γ)⁵Li capture at astrophysical energy and its role in accumulation of 6Li at the BBN

NUCLEAR REACTIONS ³H(³He, γ)⁶Li;³He(d, γ)⁵Li;⁵Li(n, γ)⁶Li, E=0-5 MeV (T below 10 GK); calculated, analyzed reaction rates; deduced assumption that two-step processes ³He(d, γ)⁵Li+γ and ⁵Li(n, γ)⁶Li+γ can make a significant contribution to ⁶Li formation at Big Bang Nucleosynthesis (BBN) at least at temperatures of the order of 1 GK; calculated total σ, astrophysical S-factor, reaction rates using modified potential cluster model with forbidden states; deduced parameters using comparison to data, presented updated compilation for ^3He(d, γ)⁵Li.

doi: 10.1016/j.nuclphysa.2019.03.017
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2011DU19      Phys.Atomic Nuclei 74, 984 (2011); Yad.Fiz. 74, 1013 (2011)

S.B.Dubovichenko, N.Burtebaev, D.M.Zazulin, Zh.K.Kerimkulov, A.S.A.Amar

Astrophysical S factor for the radiative-capture reaction p⁶Li → ⁷Beγ

NUCLEAR REACTIONS ⁶Li, ¹²C, ¹⁹F, ²⁷Al(p, γ), (p, p), E=590-1150 keV; measured reaction products, proton spectra; deduced σ(θ), S-factors. Optical model calculations, comparison with experimental data.

doi: 10.1134/S1063778811050073
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0800.

2008BU19      Phys.Rev. C 78, 035802 (2008)

N.Burtebaev, S.B.Igamov, R.J.Peterson, R.Yarmukhamedov, D.M.Zazulin

New measurements of the astrophysical S factor for ¹²C(p, γ)¹³N reaction at low energies and the asymptotic normalization coefficient (nuclear vertex constant) for the p+¹²C → ¹³N reaction

NUCLEAR REACTIONS ¹²C(p, γ), E=354, 390, 460, 463, 565, 750, 1061 keV; measured Eγ, Iγ, σ, σ(θ). Deduced astrophysical S-factors, asymptotic normalization coefficients.

doi: 10.1103/PhysRevC.78.035802
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0819.