NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = A.I.Chugunov Found 3 matches. 2013CH39 Bull.Rus.Acad.Sci.Phys. 77, 890 (2013); Izv.Akad.Nauk RAS, Ser.Fiz 77, 978 (2013) A.I.Chugunov, A.V.Afanasjev, M.Beard, M.Wiescher, D.G.Yakovlev Simple approximation of cross sections for nuclear reactions involving Z = 3-12, 14 nuclei NUCLEAR REACTIONS Be, B, C, N, O, F, Ne, Na, Mg, Si(Be, X), B, C, N, O, F, Ne, Na, Mg, Si(B, X), C, N, O, F, Ne, Na, Mg, Si(C, X), N, O, F, Ne, Na, Mg, Si(N, X), O, F, Ne, Na, Mg, Si(O, X), F, Ne, Na, Mg, Si(F, X), Ne, Na, Mg, Si(Ne, X), Na, Mg, Si(Na, X), Mg, Si(Mg, X), Si(Si, X), E not given; San Paulo potential, below the Coulomb barrier energies.
doi: 10.3103/S1062873813070083
2012AF01 Phys.Rev. C 85, 054615 (2012) A.V.Afanasjev, M.Beard, A.I.Chugunov, M.Wiescher, D.G.Yakovlev Large collection of astrophysical S factors and their compact representation NUCLEAR REACTIONS Be(Be, X), (B, X), (C, X), (N, X), (O, X), (F, X), (Ne, X), (Na, X), (Mg, X), (Si, X), B(B, X), (C, X), (N, X), (O, X), (F, X), (Ne, X), (Na, X), (Mg, X), (Si, X), C(C, X), (N, X), (F, X), (O, X), (Ne, X), (Na, X), (Mg, X), (Si, X), N(N, X), (O, X), (F, X), (Ne, X), (Na, X), (Mg, X), (Si, X), O(O, X), (F, X), (Ne, X), (Na, X), (Mg, X), (Si, X), F(F, X), (Ne, X), (Na, X), (Mg, X), (Si, X), Ne(Ne, X), (Na, X), (Mg, X), (Si, X), Na(Na, X), (Mg, X), (Si, X), Mg(Mg, X), (Si, X), Si(Si, X), E<39.8 MeV; calculated astrophysical S factors as function of incident energy for A=8-14 Be, A=9-21 for B, A=10-24 for C, A=11-27 for N, A=12-28 for O, A=17-29 for F, A=18-40 for Ne, A=19-43 for Na, A=20-46 for Mg and A=24-52 for Si for a database of 5000 nonresonant fusion reactions. Sao Paulo method and the barrier penetration model. Comparison with experimental data.
doi: 10.1103/PhysRevC.85.054615
2009CH35 Phys.Rev. C 80, 014611 (2009) Nuclear fusion reaction rates for strongly coupled ionic mixtures NUCLEAR REACTIONS 12C(16O, X), (12C, X), 16O(16O, X), E not given;calculated enhancement factors of nuclear reaction rates in the mean-field WKB approximation, effect of the plasma screening on astrophysical S factors, and Gamow-peak energies using Monte Carlo calculations of the mean-field plasma potential for strongly coupled binary ionic mixtures.
doi: 10.1103/PhysRevC.80.014611
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