NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = D.G.Yakovlev Found 17 matches. 2014KR02 Phys.Rev. C 89, 015802 (2014) Strong plasma screening in thermonuclear reactions: Electron drop model NUCLEAR REACTIONS 12C(12C, X), E not given; calculated plasma screening potentials and thermonuclear reaction rates, astrophysical S factor using newly suggested electron drop model. Non-resonant nuclear fusion in dense matter in thermonuclear regime with strong plasma screening.
doi: 10.1103/PhysRevC.89.015802
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
2012PO06 Phys.Rev. C 85, 039801 (2012) Comment on "Equation of state of a dense and magnetized fermion system"
doi: 10.1103/PhysRevC.85.039801
2012SH23 Phys.Rev. C 86, 015808 (2012) P.S.Shternin, M.Beard, M.Wiescher, D.G.Yakovlev Neutron degeneracy and plasma physics effects on radiative neutron captures in neutron star crust NUCLEAR REACTIONS 38Mg(n, γ), E<1.5 MeV; 39Mg(n, γ), E<0.1 MeV; 46Mg(n, γ), E<6 MeV; 62Ca(n, γ), E<10 MeV; calculated astrophysical σ(E), Rn ratios (Fermi-Dirac to Maxwell-Boltzmann cross sections), forward and inverse reaction rates in dense stellar medium with consideration of effects of plasma physics and neutron degeneracy in neutron star crust.
doi: 10.1103/PhysRevC.86.015808
2010BE12 At.Data Nucl.Data Tables 96, 541 (2010) M.Beard, A.V.Afanasjev, L.C.Chamon, L.R.Gasques, M.Wiescher, D.G.Yakovlev Astrophysical S factors for fusion reactions involving C, O, Ne, and Mg isotopes NUCLEAR REACTIONS C(C, X), (O, X), (Ne, X), (Mg, X), O(O, X), (Ne, X), (Mg, X), Ne(Ne, X), (Mg, X), Mg(Mg, X), E≈18-30 MeV MeV; calculated S-factors; deduced reaction rates calculation procedure.
doi: 10.1016/j.adt.2010.02.005
2010YA19 Phys.Rev. C 82, 044609 (2010) D.G.Yakovlev, M.Beard, L.R.Gasques, M.Wiescher Simple analytic model for astrophysical S factors NUCLEAR REACTIONS 46Mg(46Mg, X), E=29.9 MeV; 12C(12C, X), E=1-12 MeV; C(C, X), (O, X), E=2-17.9 MeV; C(Ne, X), (Mg, X), O(O, X), E=2-19.9 MeV; O(Ne, X), (Mg, X), Ne(Ne, X), E=2-21.9 MeV; Ne(Mg, X), E=2-24.9 MeV; Mg(Mg, X), E=2-29.9 MeV; calculated astrophysical S factors using a simple model with physically meaningful parameters. Comparison with experimental data.
doi: 10.1103/PhysRevC.82.044609
2007GA43 Phys.Rev. C 76, 035802 (2007) L.R.Gasques, E.F.Brown, A.Chieffi, C.L.Jiang, M.Limongi, C.Rolfs, M.Wiescher, D.G.Yakovlev Implications of low-energy fusion hindrance on stellar burning and nucleosynthesis NUCLEAR REACTIONS 12C, 16O(16O, X), E < 12 MeV; 16O(16O, X), E < 15 MeV; analyzed fusion cross sections. Deduced S-factors at astrophysical energies.
doi: 10.1103/PhysRevC.76.035802
2007GA50 Phys.Rev. C 76, 045802 (2007) L.R.Gasques, A.V.Afanasjev, M.Beard, J.Lubian, T.Neff, M.Wiescher, D.G.Yakovlev Sao Paulo potential as a tool for calculating S factors of fusion reactions in dense stellar matter NUCLEAR REACTIONS 16O(16O, X), E(cm)=0-20 MeV; 20O(20O, X), E=0-28 MeV; 20O(26Ne, X), E=0-20 MeV; 20O(32Mg, X), E=0-24 MeV; 26Ne(26Ne, X), E=0-24 MeV; 26Ne(32Mg, X), E=0-28 MeV; 32Mg(32Mg, X), E=0-28 MeV; 22O(22O, X), E=0-20 MeV; 24O(24O, X), E(cm)=0-20 MeV; calculated astrophysical S-factors for fusion reactions. Sao Paulo potential.
doi: 10.1103/PhysRevC.76.045802
2006YA14 Phys.Rev. C 74, 035803 (2006) D.G.Yakovlev, L.R.Gasques, A.V.Afanasjev, M.Beard, M.Wiescher Fusion reactions in multicomponent dense matter NUCLEAR REACTIONS 12C, 16O(12C, X), (16O, X), E(cm)=0-20 MeV; calculated astrophysical S-factors, fusion rates in dense matter.
doi: 10.1103/PhysRevC.74.035803
2005GA33 Phys.Rev. C 72, 025806 (2005) L.R.Gasques, A.V.Afanasjev, E.F.Aguilera, M.Beard, L.C.Chamon, P.Ring, M.Wiescher, D.G.Yakovlev Nuclear fusion in dense matter: Reaction rate and carbon burning NUCLEAR REACTIONS 12C(12C, 12C), E(cm)=6-10 MeV; calculated σ(θ). 12C(12C, X), E(cm) ≈ 0-10 MeV; calculated astrophysical S-factor, fusion rate in dense matter.
doi: 10.1103/PhysRevC.72.025806
2005YA09 Nucl.Phys. A752, 590c (2005) D.G.Yakovlev, O.Y.Gnedin, M.E.Gusakov, A.D.Kaminker, K.P.Levenfish, A.Y.Potekhin Neutron star cooling
doi: 10.1016/j.nuclphysa.2005.02.061
2005YA29 Eur.Phys.J. A 25, Supplement 1, 669 (2005) D.G.Yakovlev, K.P.Levenfish, O.Y.Gnedin Pycnonuclear reactions in dense stellar matter
doi: 10.1140/epjad/i2005-06-093-1
1995GN01 Nucl.Phys. A582, 697 (1995) Thermal Conductivity of Electrons and Muons in Neutron Star Cores
doi: 10.1016/0375-9474(94)00503-F
1993VE11 At.Data Nucl.Data Tables 55, 233 (1993) D.A.Verner, D.G.Yakovlev, I.M.Band, M.B.Trzhaskovskaya Subshell Photoionization Cross Sections and Ionization Energies of Atoms and Ions from He to Zn ATOMIC PHYSICS Z=4-30; calculated subshell partial photoionization σ.
doi: 10.1006/adnd.1993.1022
1985MA61 Izv.Akad.Nauk SSSR, Ser.Fiz. 49, 2150 (1985); Bull.Acad.Sci.USSR, Phys.Ser. 49, No.11, 61 (1985) Calculation of the Neutron s-Wave Strength Function in the Odd Yb, Hf, W and Os Isotopes NUCLEAR STRUCTURE 175,177Yb, 179,181Hf, 181,183,185W, 187Os; calculated s-wave strength function.
1985MA62 Izv.Akad.Nauk SSSR, Ser.Fiz. 49, 2187 (1985); Bull.Acad.Sci.USSR, Phys.Ser. 49, No.11, 97 (1985) Calculation of the Neutron s-Wave Strength Function of the Even Hf and W Isotopes NUCLEAR STRUCTURE 178,180Hf, 182,184W; calculated s-wave neutron strength function. Quasiparticle-phonon model.
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