Ab initio nucleon-nucleus elastic scattering with chiral effective field theory uncertainties
arXiv:2112.02442 · doi:10.1103/PhysRevC.106.064605
Abstract
Background: Effective interactions for nucleon-nucleus () elastic scattering from first principles require the use of the same nucleon-nucleon () interaction in the structure and reaction calculations, and a consistent treatment of the relevant operators at each order. Purpose: Truncation uncertainties of chiral forces have been studied for scattering observables in few-body systems and for bound state properties of light nuclei. We extend this to elastic scattering. Methods: With the spectator expansion of multiple scattering theory and the no-core shell model, we use a chiral interaction from the LENPIC collaboration to consistently calculate the leading order effective interaction up to third chiral order (N2LO) and extract elastic scattering observables. We quantify the chiral truncation error using pointwise and correlated methods. Results: We analyze proton-O and neutron-C elastic scattering observables between 65 and 185 MeV projectile kinetic energy. We find qualitatively similar results for the chiral truncation uncertainties as in few-body systems, which we assess using similar diagnostic tools. The order-by-order convergence of the scattering observables for O and C is reasonable near 100 MeV, but for higher energies the expansion parameter becomes too large to converge. We find a near-perfect correlation between the neutron differential cross section and the Wolfenstein amplitudes for small momentum transfers. Conclusions: The tools used to study the convergence of a chiral interaction in few-body systems can be applied to scattering with minor changes. The interaction used here gives a good description of O and C scattering observables as low as 65 MeV. The very forward direction of the neutron differential cross section mirrors the behavior of the interaction amazingly well.
arXiv comment17 pages, 13 figures, 1 table
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