NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = P.Fachini Found 11 matches. 2009FA11 Nucl.Phys. A830, 837c (2009) P.Fachini, and the STAR collaboration ρ0 Production in Cu+Cu Collisions at √ sNN = 200 GeV and 62.4 GeV in STAR
doi: 10.1016/j.nuclphysa.2009.10.007
2007FA01 J.Phys.(London) G34, 431 (2007) P.Fachini, R.S.Longacre, Z.Xu, H.Zhang Indication for π+π- scattering in p + p collisions at √ sNN = 200 GeV NUCLEAR REACTIONS 1H(p, X), E(cm)=200 GeV; analyzed ρ0 production associated invariant mass spectra; deduced contribution from pion scattering interactions.
doi: 10.1088/0954-3899/34/3/002
2004FA01 J.Phys.(London) G30, S565 (2004) P.Fachini, for the STAR Collaboration ρ(770)0 and f0(980) production in Au + Au and pp collisions at √ sNN = 200 GeV NUCLEAR REACTIONS 197Au(197Au, X), E(cm)=200 GeV/nucleon; 1H(p, X), E(cm)=200 GeV; measured resonance production associated invariant mass spectra, transverse momentum, yields. Comparison with model predictions.
doi: 10.1088/0954-3899/30/1/069
2004FA17 Acta Phys.Pol. B35, 183 (2004) Resonance Production in Au+Au and p+p Collisions at √ sNN = 200 GeV NUCLEAR REACTIONS 1H(p, X), 197Au(197Au, X), E(cm)=200 GeV/nucleon; analyzed resonance yield ratios, transverse momentum, related data; deduced phase space and dynamical effects.
2004FA22 J.Phys.(London) G30, S735 (2004) Resonance production
doi: 10.1088/0954-3899/30/8/012
2003FA04 Nucl.Phys. A715, 462c (2003) P.Fachini, and the STAR Collaboration p(770)0, K*(892)0 and f0(980) Production in Au-Au and pp Collisions at √ sNN=200 GeV NUCLEAR REACTIONS 1H(p, X), 197Au(197Au, X), E(cm)=200 GeV/nucleon; measured resonance production associated invariant mass spectra, yield ratios.
doi: 10.1016/S0375-9474(02)01444-6
2002FA06 J.Phys.(London) G28, 1599 (2002) P.Fachini, for the STAR Collaboration K*(892)0 Production in Relativistic Heavy-Ion Collisions at √ SNN = 130 GeV NUCLEAR REACTIONS 197Au(197Au, X), E(cm)=130 GeV; measured K*0 production associated invariant mass, yields. Mixed-event technique.
doi: 10.1088/0954-3899/28/7/311
2002FA20 Acta Phys.Hung.N.S. 15, 195 (2002) P.Fachini, and the STAR Collaboration Resonance Studies at STAR NUCLEAR REACTIONS 197Au(197Au, X), E(cm)=130 GeV/nucleon; measured resonance production associated invariant mass spectra, particle yield ratios.
doi: 10.1556/APH.15.2002.3-4.3
1997SC14 Nucl.Phys. A620, 91 (1997) W.Sciani, A.Lepine-Szily, R.Lichtenthaler, P.Fachini, L.C.Gomes, G.F.Lima, M.M.Obuti, J.M.Oliveira, Jr., A.C.C.Villari The 12C + 24Mg Elastic Scattering: An example of anomalous transparency at Coulomb barrier energies NUCLEAR REACTIONS 24Mg(12C, 12C), (12C, 12C'), E(cm)=10.67-16 MeV; measured σ(θ); deduced model parameters energy dependence. Coupled channels approach.
doi: 10.1016/S0375-9474(97)00157-7
1996OL02 Phys.Rev. C53, 2926 (1996) J.M.Oliveira, Jr., A.Lepine-Szily, A.C.C.Villari, R.Lichtenthaler, L.C.Gomes, W.Sciani, P.Fachini, G.L.Lima, A.C.G.Martins, V.Chiste, J.M.Casandjian, A.J.Pacheco, J.E.Testoni, D.Abriola, A.O.Macchiavelli, F.Hasenbalg, O.A.Capurro, D.Tomasi, J.Fernandez Niello, D.Brandizzi Orbiting Features in the Strongly Damped Binary Decay of the 28Si + 16O System NUCLEAR REACTIONS 16O(28Si, 28Si), (28Si, 32S), (28Si, 24Mg), E=107.5, 139 MeV; measured σ(θ), emitted particles mass distribution; deduced optical model parameters, reaction mechanism. Coupled-channels analysis.
doi: 10.1103/PhysRevC.53.2926
1992LE04 Nucl.Phys. A539, 487 (1992) A.Lepine-Szily, J.M.Oliveira, Jr., P.Fachini, R.Lichtenthaler Filho, M.M.Obuti, W.Sciani, M.K.Steinmayer, A.C.C.Villari Orbiting in the Algebraic Scattering Framework NUCLEAR REACTIONS 10,11B(18O, 18O), (18O, 14C), E(cm)=18.8, 19.9 MeV; measured σ(θ). Coupled-channels calculations using algebraic scattering theory.
doi: 10.1016/0375-9474(92)90289-V
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