Ab initio folding potentials for nucleon-nucleus scattering based on no-core shell-model one-body densities

M. Burrows, Ch. Elster, S. P. Weppner, K. D. Launey, P. Maris, A. Nogga, and G. Popa
Phys. Rev. C 99, 044603 – Published 15 April 2019

Abstract

Background: Calculating microscopic optical potentials for elastic nucleon-nucleus scattering has already led to large body of work in the past. For folding first-order calculations the nucleon-nucleon (NN) interaction and the one-body density of the nucleus were taken as input to rigorous calculations in a spectator expansion of the multiple scattering series.

Purpose: Based on the Watson expansion of the multiple scattering series we employ a nonlocal translationally invariant nuclear density derived from a chiral next-to-next-to-leading order (NNLO) and the very same interaction for consistent full-folding calculation of the effective (optical) potential for nucleon-nucleus scattering for light nuclei.

Methods: The first order effective (optical) folding potential is computed by integrating over the nonlocal, translationally invariant NCSM one-body density and the off-shell Wolfenstein amplitudes A and C. The resulting nonlocal potential serves as input for a momentum-space Lippmann-Schwinger equation, whose solutions are summed to obtain the nucleon-nucleus scattering observables.

Results: We calculate scattering observables, such as total, reaction, and differential cross sections as well as the analyzing power and the spin-rotation parameter, for elastic scattering of protons and neutrons from He4, He6, C12, and O16, in the energy regime between 100 and 200 MeV projectile kinetic energy, and compare to available data.

Conclusions: Our calculations show that the effective nucleon-nucleus potential obtained from the first-order term in the spectator expansion of the multiple scattering expansion describes experiments very well to about 60 degrees in the center-of-mass frame, which coincides roughly with the validity of the NNLO chiral interaction used to calculate both the NN amplitudes and the one-body nuclear density.

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  • Received 16 October 2018

DOI:https://doi.org/10.1103/PhysRevC.99.044603

©2019 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. Burrows1, Ch. Elster1, S. P. Weppner2, K. D. Launey3, P. Maris4, A. Nogga5, and G. Popa1

  • 1Institute of Nuclear and Particle Physics, and Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
  • 2Natural Sciences, Eckerd College, St. Petersburg, Florida 33711, USA
  • 3Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
  • 4Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
  • 5IAS-4, IKP-3, JHCP, and JARA-HPC, Forschungszentrum Jülich, D-52428 Jülich, Germany

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Vol. 99, Iss. 4 — April 2019

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