M1 Resonances in Unstable Magic Nuclei
arXiv:nucl-th/9303001 · doi:10.1007/BF01292513
Abstract
Within a microscopic approach which takes into account RPA configurations, the single-particle continuum and more complex configurations isoscalar and isovector M1 excitations for the unstable nuclei Ni and Sn are calculated. For comparison, the experimentally known M1 excitations in Ca and Pb have also been calculated. In the latter nuclei good agreement in the centroid energy, the total transition strength and the resonance width is obtained. With the same parameters we predict the magnetic excitations for the unstable nuclei. The strength is sufficiently concentrated to be measurable in radioactive beam experiments. New features are found for the very neutron rich nucleus Ni and the neutron deficient nucleus Sn.
17 pages (LATEX), 12 figures (available from the authors), KFA-IKP(TH)-1993-07
Cited by in corpus (14)
- Extended Theory of Finite Fermi Systems (Collective Vibrations in Closed Shell Nuclei)
- Gamow-Teller Strength in the Region of Sn
- Microscopic description of the pygmy and giant electric dipole resonances in stable Ca isotopes
- Magnetic dipole excitations based on the relativistic nuclear energy density functional
- Low-energy M1 excitations in Pb and the spin channel of the Skyrme energy-density functional
- Measurements of the 48Ca(γ,n) Reaction
- Self-consistent calculations within the Extended Theory of Finite Fermi Systems
- M1 resonance in Pb within the self-consistent phonon-coupling model
- Role of residual interaction in the relativistic description of M1 excitation
- Optimizing phonon space in the phonon-coupling model
- Magnetic dipole excitation and its sum rule in nuclei with two valence nucleons
- The evolution of magnetic dipole strength in Sn isotope chain and quenching of nucleon g factors
- Isovector spin susceptibility: Isotopic evolution of collectivity in spin response
- Magnetic quadrupole transitions in the relativistic energy density functional theory