Abstract
We perform a detailed comparison of results of the Gamow Shell Model (GSM) and the Gaussian Expansion Method (GEM) supplemented by the complex scaling (CS) method for the same translationally-invariant cluster-orbital shell model (COSM) Hamiltonian. As a benchmark test, we calculate the ground state and the first excited state of mirror nuclei He and Be in the model space consisting of two valence nucleons in -shell outside of a He core. We find a good overall agreement of results obtained in these two different approaches, also for many-body resonances.
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