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With a view toward describing reactions of intermediate-mass nuclei fromfirst principles, we present first results for the norm and Hamiltonianoverlaps (kernels) for the p-{\alpha}, p-16O and p-20Ne cluster systems usingrealistic nucleon-nucleon interactions. This is achieved in the framework of anew ab initio approach that combines the symmetry-adapted no-core shell model(SA-NCSM) with the resonating group method (RGM). In this model, a physicallyrelevant basis based on the SU(3) symmetry is used. The structure of theclusters is provided by the ab initio SA-NCSM, which enables the description ofspatially enhanced nuclear configurations and heavier nuclei, by exploitingsymmetries known to dominate in nuclei. Here, we discuss the applicability andefficacy of this approach.

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