NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = G.K.Matushko Found 4 matches. 2006KO02 Phys.Atomic Nuclei 69, 120 (2006) V.B.Kopeliovich, A.M.Shunderuk, G.K.Matushko Mass Splittings of Nuclear Isotopes in Chiral Soliton Approach NUCLEAR STRUCTURE 6H, 8,9,10He, 6,10,11,12Li, 8,9,10,12,13,14,15,16,17Be, 10,11,12,14,15,16,17,18,19B, 12,13,14,15,16,17,18,19,20,21C, 14,15,16,17,18,19,20,21,22,23N, 16,17,18,19,20,21,22,23,24,25O, 18,19,20,21,22,23,24,25,26,27F, 20,21,22,23,24,25,26,27,28,29Ne, 22,23,24,25,26,27,28,29,30,31Na, 24,25,26,27,28,29,30,31,32Mg, 26,27,28,29,30,31,32Al, 28,29,30,31,32Si, 30,31,32P, 32S; analyzed binding energy differences. 17Li, 18,19Be, 20,21B, 22,23C, 24,25N, 26,27O, 28,29F, 30,31Ne, 32Na; calculated binding energies. Chiral soliton approach.
doi: 10.1134/S1063778806010169
1998KA20 Yad.Fiz. 61, No 3, 409 (1998); Phys.Atomic Nuclei 61, 349 (1998) M.V.Kazarnovsky, V.L.Matushko, G.K.Matushko, V.G.Miroshnichenko, S.A.Novoselov, Yu.P.Popov, P.V.Sedyshev, M.V.Sedysheva, O.A.Langer New Method for Generating Fluxes of Neutrons Having Maxwell Spectra Characterized by Temperatures of 10-40 keV for Direct Measurements of the Cross Section for Neutron Capture in the Stellar s Process NUCLEAR REACTIONS 3H, 7Li(p, n), E not given; calculated σ(En). Design of neutron source for capture measurements.
1997KA44 Nucl.Phys. A621, 239c (1997) M.V.Kazarnovsky, O.A.Langer, G.K.Matushko, V.L.Matushko, V.G.Miroshnichenko, S.V.Novoseolov, Yu.P.Popov, M.V.Sedysheva A New Method for Generating in a Moderator the Maxwellian Neutron Spectra for Stellar Temperatures
doi: 10.1016/S0375-9474(97)00245-5
1983RY02 Z.Phys. A311, 363 (1983) Yu.V.Ryabov, G.K.Matushko, V.N.Slastnikov Measurement of the Average Neutrons Yield from 250 MeV Protons Absorbed in a Lead Target NUCLEAR REACTIONS Pb(p, n), E=250 MeV; measured thick target yields.
doi: 10.1007/BF01415692
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