Comparison of Relativistic Nucleon-Nucleon Interactions
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We investigate the difference between those relativistic models based on interpreting a realistic nucleon-nucleon interaction as a perturbation of the square of a relativistic mass operator and those models that use the method of Kamada and Gl\"ockle to construct an equivalent interaction to add to the relativistic mass operator. Although both models reproduce the phase shifts and binding energy of the corresponding non-relativistic model, they are not scattering equivalent. The example of elastic electron-deuteron scattering in the one-photon-exchange approximation is used to study the sensitivity of three-body observables to these choices. Our conclusion is that the differences in the predictions of the two models can be understood in terms of the different ways in which the relativistic and non-relativistic $S$-matrices are related. We argue that the mass squared method is consistent with conventional procedures used to fit the Lorentz-invariant cross section as a function of the laboratory energy.
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Coarse graining hadronic scattering
Coarse graining of hadronic scattering fixes long-range chiral dynamics above cutoff r_c and counts short-range parameters as N_Par = N_S × N_I × (p r_c)^2 / 2 for χ² fits with proper degrees of freedom.
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