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Spectroscopic factors involving well bound nucleons in light nuclei arecalculated with standard shell model, no-core shell model and Gamow shellmodel. Continuum coupling is included exactly in the Gamow shell model, due tothe use of the Berggren basis, which contains bound, resonance and scatteringstates. Conversely, it is absent from standard and no-core shell models, wherea basis of harmonic oscillator states is used. As the A - 1 nuclei for whichspectroscopic factors are calculated are either weakly bound or unbound,coupling to continuum is prominent, even though the A nuclei are well bound. Itis then showed that Gamow shell model can properly reproduce experimental dataand is a predictive tool for detailed nuclear structure at drip-line, contraryto standard and no-core shell model.

Investigation of spectroscopic factors of deeply-bound nucleons in drip-line nuclei with the Gamow shell model