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 many-particle (quasi-)bound states and the continuum of one-particle scattering states to the spectroscopy of 8B and to the calculation of astrophysical factors in the reaction 7Be(p,gamma)8B.

9 pages incl. 3 figures, LaTeX with iopart class and epsf. Invited talk at the Int. Workshop on Physics with Radioactive Nuclear Beams, Jan. 12-17, 1998, Puri, India. Shortened version will be published in proceedings to apear as a separate J. Phys. G volume

Cited by in corpus (12)

• Radioactive decays at limits of nuclear stability
• Shell Model in the Complex Energy Plane
• Study of the ${}^{7}Be(p,\gamma {)}^{8}B$ and ${}^{7}Li(n,\gamma {)}^{8}Li$ capture reactions using the shell model embedded in the continuum
• Low energy measurement of the 7Be(p,gamma)8B cross section
• Analysis of the 16O(p,gamma)17F capture reaction using the shell model embedded in the continuum
• Continuum effects for the mean-field and pairing properties of weakly bound nuclei
• New Discrete Basis for Nuclear Structure Studies
• First-forbidden mirror beta-decays in A=17 mass region
• Gamow Shell Model description of Li isotopes and their mirror partners
• Description of the 17F(p,gamma)18Ne radiative capture reaction in the continuum shell model
• Role of spectroscopic factors in the potential-model description of the Be7(p,gamma)B8 reaction
• Structure effects on the Coulomb dissociation of 8B at relativistic energies