NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = S.G.Matinyan Found 6 matches. 1998MA15 Phys.Rev. C57, 1927 (1998) S.G.Matinyan, B.Muller, D.H.Rischke Classical Gluon Radiation in Ultrarelativistic Nuclear Collisions: Space-time structure, instabilities, and thermalization
doi: 10.1103/PhysRevC.57.1927
1998MA73 Phys.Rev. C58, 2994 (1998) Model of Charmonium Absorption by Light Mesons
doi: 10.1103/PhysRevC.58.2994
1997MA49 Phys.Rev. C56, 2191 (1997) S.G.Matinyan, B.Muller, D.H.Rischke Gluon Radiation and Coherent States in Ultrarelativistic Nuclear Collisions
doi: 10.1103/PhysRevC.56.2191
1995BI18 Phys.Lett. 362B, 29 (1995) T.S.Biro, S.G.Matinyan, B.Muller Chaos Driven by Soft-Hard Mode Coupling in Thermal Yang-Mills Theory
doi: 10.1016/0370-2693(95)01205-5
1989AR02 Yad.Fiz. 49, 86 (1989) T.A.Arakelyan, L.S.Davtyan, S.G.Matinyan Quark Degrees of Freedom and Photoabsorption of Nuclei NUCLEAR STRUCTURE 2H, 6Li, 9Be, 12C, 16O, 27Al, 40Ca, 118Sn, 133Cs, 180Ta, 208Pb, 235U; calculated E1 photoabsorption sum rule; deduced six quark configuration role.
1986AZ02 Yad.Fiz. 44, 446 (1986); Sov.J.Nucl.Phys. 44, 286 (1986) I.G.Aznauryan, L.S.Davtyan, A.T.Margaryan, S.G.Matinyan Electric Dipole Photoabsorption and the Quark Structure of Nucleons NUCLEAR REACTIONS 1H(γ, π+), (γ, π-), E=1.2 GeV; calculated E1 photoabsorption σ vs transition energy; deduced E1 photoabsorption sum rules. Constitutent-quark model.
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