Low-energy pd scattering: High-precision data, comparisons with theory, and phase-shift analyses

M. H. Wood, C. R. Brune, B. M. Fisher, H. J. Karwowski, D. S. Leonard, E. J. Ludwig, A. Kievsky, S. Rosati, and M. Viviani
Phys. Rev. C 65, 034002 – Published 8 February 2002
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Abstract

Angular distributions of σ(θ), Ay, iT11, T20, T21, and T22 have been measured for dp 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 pd and nd 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.

  • Received 5 October 2001

DOI:https://doi.org/10.1103/PhysRevC.65.034002

©2002 American Physical Society

Authors & Affiliations

M. H. Wood*, C. R. Brune, B. M. Fisher, H. J. Karwowski, D. S. Leonard, and E. J. Ludwig

  • Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, North Carolina 27599-3255
  • Triangle Universities Nuclear Laboratory, Durham, North Carolina 27088-0308

A. Kievsky, S. Rosati, and M. Viviani

  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa and Dipartimento di Pisa, Universita di Pisa, I-56100 Pisa, Italy

  • *Present address: Thomas Jefferson National Accelerator Facility, 12000 Jefferson Ave., Newport News, VA 23606.
  • Present address: Department of Physics and Astronomy, Ohio University, Athns, OH 45701.

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Vol. 65, Iss. 3 — March 2002

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