NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = S.A.Turakulov Found 8 matches. 2023TU06 Phys.Rev. C 108, 065801 (2023) E.M.Tursunov, S.A.Turakulov, K.I.Tursunmakhatov Detailed study of the astrophysical direct capture reaction 6Li(p, γ)7Be in a potential model approach
doi: 10.1103/PhysRevC.108.065801
2021TU01 Nucl.Phys. A1006, 122108 (2021) E.M.Tursunov, S.A.Turakulov, A.S.Kadyrov Analysis of the 3He(α, γ)7Be and 3H(α, γ)7Li astrophysical direct capture reactions in a modified potential-model approach NUCLEAR REACTIONS 3He(α, γ), 3H(α, γ), E(cm)<8 MeV; analyzed available data; deduced S-factors, contributions of the E1, E2 and M1 astrophysical S factors, reaction rates in the framework of a modified two-body potential model.
doi: 10.1016/j.nuclphysa.2020.122108
2021TU04 Phys.Rev. C 104, 045806 (2021) E.M.Tursunov, S.A.Turakulov, A.S.Kadyrov, L.D.Blokhintsev Astrophysical S factor and rate of 7Be (p, γ)8B direct capture reaction in a potential model NUCLEAR REACTIONS 7Be(p, γ)8B, E(cm)<13 MeV; calculated s-wave-scattering length, phase shift, astrophysical S factor, partial E1, E2, and M1 components of astrophysical S factor. 7Be(p, γ)8B, T9=0.001-10.0; calculated capture reaction rates. Comparison of astrophysical S factor with experimental data, and reaction rates with the results of the NACRE II Collaboration. Two-body potential model using single-channel approximation, with a modified potential.
doi: 10.1103/PhysRevC.104.045806
2020TU03 Nucl.Phys. A1000, 121884 (2020) E.M.Tursunov, S.A.Turakulov, A.S.Kadyrov Comparative study of the direct α + d → 6Li + γ astrophysical capture reaction in few-body models
doi: 10.1016/j.nuclphysa.2020.121884
2018TU04 Phys.Rev. C 97, 035802 (2018) E.M.Tursunov, S.A.Turakulov, A.S.Kadyrov Astrophysical 3He(α, γ)7Be and 3H(α, γ)7Li direct capture reactions in a potential-model approach NUCLEAR REACTIONS 3He, 3H(α, γ), E(cm)<6 MeV; calculated s-wave phase-shifts, contributions of the partial and total E1, E2, and M1 components to the astrophysical S factor, astrophysical S factor using two-body potential model with potentials of a simple Gaussian form. Comparison with experimental data from LUNA collaboration, and other studies.
doi: 10.1103/PhysRevC.97.035802
2018TU11 Phys.Rev. C 98, 055803 (2018) E.M.Tursunov, S.A.Turakulov, A.S.Kadyrov, I.Bray Theoretical study of the α + d → 6Li + γ astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance NUCLEAR REACTIONS 2H(α, γ)6Li, E=0.01-3 MeV; calculated partial E1 and E2 astrophysical S factors, overlap integral, astrophysical reaction rate in 0.001 to 10 GK range, and primordial 6Li abundance using three body model. Comparison with experimental data from LUNA Collaboration, and from NACRE 1999 database.
doi: 10.1103/PhysRevC.98.055803
2016TU06 Phys.Rev. C 94, 015801 (2016) E.M.Tursunov, A.S.Kadyrov, S.A.Turakulov, I.Bray Theoretical study of the α + d → 6Li + γ astrophysical capture process in a three-body model NUCLEAR REACTIONS 2H(α, γ)6Li, E=0.05-3 MeV; calculated contribution of E1-transition operator from the isosinglet states to the isotriplet components of the final 6Li(1+) bound state, astrophysical S(E) factors and compared with experimental data from the LUNA Collaboration. Three-body (α+n+p) model with hyperspherical Lagrange-mesh method.
doi: 10.1103/PhysRevC.94.015801
2015TU03 Phys.Atomic Nuclei 78, 193 (2015) E.M.Tursunov, S.A.Turakulov, P.Descouvemont Theoretical analysis of the astrophysical S-factor for the capture reaction α+d → 6Li + γ in the two-body model NUCLEAR REACTIONS 2H(α, γ), E<12 MeV; analyzed available data; deduced S-wave phase shifts, Contributions of E1, E2, and E1+E2 transitions to the astrophysical S-factor, theoretical estimate for reaction rates.
doi: 10.1134/S1063778815010196
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