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arXiv · 1910.00638

New symmetry-adapted ab initio approach to nuclear reactions for intermediate-mass nuclei

Alexis Mercenne·Kristina D. Launey·Jutta E. Escher·Tomas Dytrych·Jerry P. Draayer
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Abstract

With a view toward describing reactions of intermediate-mass nuclei from first principles, we present first results for the norm and Hamiltonian overlaps (kernels) for the p-{\alpha}, p-16O and p-20Ne cluster systems using realistic nucleon-nucleon interactions. This is achieved in the framework of a new ab initio approach that combines the symmetry-adapted no-core shell model (SA-NCSM) with the resonating group method (RGM). In this model, a physically relevant basis based on the SU(3) symmetry is used. The structure of the clusters is provided by the ab initio SA-NCSM, which enables the description of spatially enhanced nuclear configurations and heavier nuclei, by exploiting symmetries known to dominate in nuclei. Here, we discuss the applicability and efficacy of this approach.

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Alexis Mercenne, Kristina D. Launey, Jutta E. Escher, Tomas Dytrych, Jerry P. Draayer. 2019-10-01. New symmetry-adapted ab initio approach to nuclear reactions for intermediate-mass nuclei. https://arxiv.org/abs/1910.00638

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