Natural orbital description of the halo nucleus 6He
arXiv:1605.04976 · doi:10.1007/s41365-017-0332-6
Abstract
Ab initio calculations of nuclei face the challenge of simultaneously describing strong short-range internucleon correlations and the long-range properties of weakly-bound halo nucleons. Natural orbitals, which diagonalize the one-body density matrix, provide a basis which is better matched to the physical structure of the many-body wave function. We demonstrate that the use of natural orbitals significantly improves convergence for ab initio no-core configuration interaction calculations of the neutron halo nucleus 6He, relative to the traditional oscillator basis.
6 pages, 4 figures; presented at the Symposium on Nuclear Dynamics and Thermodynamics, Huizhou, China, December 11, 2016; as published in Nucl. Sci. Tech
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- Three-cluster dynamics within the ab initio no-core shell model with continuum: How many-body correlations and -clustering shape He
- Robust ab initio prediction of nuclear electric quadrupole observables by scaling to the charge radius
- Natural orbitals for the ab initio no-core configuration interaction approach
- Intrinsic operators for the translationally-invariant many-body problem
- Uncertainties in ab initio nuclear structure calculations with chiral interactions
- Two-dimensional extrapolation procedure for ab initio study of nuclear size parameters and the properties of halo nucleus 6He
- Perspectives on Nuclear Structure and Scattering with the Ab Initio No-Core Shell Model
- Sub Coulomb barrier d+Pb scattering in the time-dependent basis function approach