McEachran, RobertStauffer, A D2015-12-130953-4075http://hdl.handle.net/1885/72402We present results based upon our ab initio relativistic optical potential method for the simulation of positronium formation in the noble gases neon, argon, krypton and xenon. The method used in this simulation is based upon an approach, first suggestedKeywords: Differential cross section; Energy regions; Ionization cross section; Ionization thresholds; Optical potential; Positronium formation; Small scattering angles; Theoretical approach; Binding energy; Experiments; Inert gases; Ionization of gases; Positrons201310.1088/0953-4075/46/7/0752032016-02-24