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Angular distributions of σ(θ), Ay, iT₁₁, T₂₀, T₂₁, and T₂₂ have been measured for d-p scattering at Ec.m.=667keV. This set of high-precision data is compared to variational calculations with the nucleon-nucleon potential alone and also to calculations including a three-nucleon $(3N)$ potential. Agreement with cross section and tensor analyzing power data is excellent when a $3N$ potential is used. However, a comparison between the vector analyzing powers reveals differences of approximately 40% in the maxima of the angular distributions which is larger than reported at higher energies for both p-d and n-d scattering. The inclusion of phenomenological spin-orbit forces in a $3N$ potential improves the comparison with vector analyzing powers substantially. Single-energy phase-shift analyses were performed on this data set and a similar data set at Ec.m.=431.3keV. The role of the different phase-shift parameters in fitting these data is discussed.
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Wood et al. (2002) studied this question.
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