From Super-Radiance to Continuum Shell Model

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Consideration of marginally stable mesoscopic systems, including nuclei on the verge of stability, requires that intrinsic structure and continuum effects be taken on equal footing. In two lectures we discuss a possible way to the continuum shell model. The approach is based on the consistent use of the effective non-Hermitian energy-dependent Hamiltonian that allows one to calculate the discrete spectrum in agreement with conventional shell model along with the reaction cross sections. We explain physics of super-radiance and trapping and show examples of first applications to long chains of neutron-rich isotopes.

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