1996/05/13 by J. F. Amundson, J.F. Amundson, O. J. P. Eboli +4 · 2 citations
Physics and Astronomy · #Crystallography and Radiation Phenomena #High-Energy Particle Collisions Research #Particle physics theoretical and experimental studies #hep-ph
paper · pdf · doi:10.1016/s0370-2693(96)01417-7
published as Phys.Lett. B390 (1997) 323-328 · 12 pages (with embedded figures), Latex2.09, uses epsf.sty and epsfig.sty. Z-compressed postscript version also available at http://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-942.ps.Z or at ftp://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-942.ps.Z
arxiv created 1996/05/13 · openalex publication_date 1997/01/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
The color evaporation model simply states that charmonium production is described by the same dynamics as D D production, \em i.e., by the formation of a colored c c pair. Its color happens to be bleached by soft final-state interactions. We show that the model gives a complete picture of charmonium production including low-energy production by proton, photon and antiproton beams, and high-energy production at the Tevatron and HERA. Our analysis includes the first next-to-leading-order calculation in the color evaporation model.