Abstract
New experimental cross-section and vector-analyzing-power data for three star configurations of the kinematically complete breakup reaction 2H(p, pp)n are compared to the rigorous Faddeev calculations involving four realistic NN potentials — Argonne AV14, Bonn B, Nijmegen and Paris. A satisfactory agreement between theory and experiment has been found. The effects of the Tucson-Melbourne three-body force included in the calculations are also discussed.KeywordsCoulomb ForceBreakup ReactionTriton Binding EnergyOutgoing NucleonElastic Scatter Cross SectionThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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