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Title: Spin-Isospin Giant Resonances and the Neutron Skin of Nuclei

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2140648· OSTI ID:20719712
 [1];  [2]; ;  [3]
  1. Physics Department, Faculty of Science, University of Zagreb (Croatia)
  2. Institut fuer Kernphysik, Technische Universitaet Darmstadt, 64289 Darmstadt (Germany)
  3. Physik-Department der Technischen Universitaet Muenchen, D-85748 Garching (Germany)

The self-consistent relativistic proton-neutron quasiparticle random phase approximation (PN-RQRPA) has been employed in the analysis of charge-exchange modes: isobaric analog states (IAS) and Gamow-Teller resonances (GTR). A particularly interesting application is the study of the relation between the neutron skin of nuclei and the difference of excitation energies of the GTR and IAS. In addition to important information on basic nuclear structure, effective isovector interactions, and neutron-rich matter for astrophysical applications, the determination of neutron density distributions is crucial for the analysis of atomic parity-violating experiments. Detailed PN-RQRPA calculations of nuclear properties of a sequence of Sn isotopes, have shown that the isotopic dependence of the energy spacings between the GTR and IAS provides a measure of the evolution of the difference between the radii of the neutron and proton density distributions.

OSTI ID:
20719712
Journal Information:
AIP Conference Proceedings, Vol. 802, Issue 1; Conference: ENS'05: International symposium on exotic nuclear systems, Debrecen (Hungary), 20-25 Jun 2005; Other Information: DOI: 10.1063/1.2140648; (c) 2005 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English