Ab initio folding potentials for nucleon-nucleus scattering based on no-core shell-model one-body densities
Ab initio folding potentials for nucleon-nucleus scattering based on no-core shell-model one-body densities
复制标题
基于无核壳模型单体密度的核子-核散射的从头计算折叠势
DOI:
10.1103/physrevc.99.044603
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发表时间:
2019
影响因子:
3.1
通讯作者:
Popa, G.
中科院分区:
文献类型:
--
作者:
Burrows, M.;Elster, Ch.;Weppner, S. P.;Launey, K. D.;Maris, P.;Nogga, A.;Popa, G.
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 () 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,,, and, 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 theamplitudes and the one-body nuclear density.