NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = G.Pech Found 4 matches. 1998AG01 Phys.Rev. C57, 953 (1998) C.E.Aguiar, T.Kodama, R.A.M.S.Nazareth, G.Pech String Mechanism for the Leading Charm Effect NUCLEAR REACTIONS 1H(p, X), (π-, X), E=high; analyzed data; deduced strong color fields, charm production related features. Flux tube picture.
doi: 10.1103/PhysRevC.57.953
1998AG10 Nucl.Phys. A638, 547c (1998) C.E.Aguiar, T.Kodama, R.A.M.S.Nazareth, G.Pech Leading Charm in Color Flux Tube
doi: 10.1016/S0375-9474(98)00376-5
1998CH07 Phys.Rev. C57, 847 (1998) K.C.Chung, C.S.Wang, A.J.Santiago, G.Pech Transverse and Forward Energy Distributions in Ultrarelativistic Heavy Collisions by an Absorption Model NUCLEAR REACTIONS Ag, Cu(16O, X), E=60 GeV/nucleon; Pb(208Pb, X), E=158 GeV/nucleon; 197Au(16O, X), E=60, 200 GeV/nucleon; S, Cu, Ag, 197Au(32S, X), E=200 GeV/nucleon; analyzed transverse, forward energy distributions; deduced parameters. Absorption model.
doi: 10.1103/PhysRevC.57.847
1996AG01 Phys.Rev. C53, 448 (1996) C.E.Aguiar, T.Kodama, R.A.M.S.Nazareth, G.Pech Charm Production in Flux Tubes NUCLEAR REACTIONS 1H(p, X), E=high; calculated charm production σ. 1H(p, X), E at 400 GeV/c; calculated charm particles x(F) distribution. 1H(p, X), E at 205 GeV/c; calculated strange particles x(F) distribution. Flux tube model.
doi: 10.1103/PhysRevC.53.448
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