A study of nuclei of astrophysical interest in the continuum shell model
Abstract
We present here the first application of realistic shell model (SM) including coupling between-particle (quasi-)bound states and the continuum of one-particle scattering states of the spectroscopy of $^{8}$B and to the calculation of astrophysical factors in the reaction $^{7}$Be(p,$\gamma$)$^{8}$B.