NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 27, 2024.

Search: Author = A.I.Chugunov

Found 3 matches.

Back to query form

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2009CH35      Phys.Rev. C 80, 014611 (2009)

A.I.Chugunov, H.E.DeWitt

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
Citations: PlumX Metrics