Pygmy Dipole Strength in Exotic Nuclei and the Equation of State
- GSI Helmholtzzentrum fuer Schwerionenforschung GmbH, Darmstadt (Germany)
- Poland
- University of Zagreb (Croatia)
A concentration of dipole strength at energies below the giant dipole resonance was observed in neutron-rich nuclei around {sup 132}Sn in an experiment using the FRS-LAND setup. This so-called 'pygmy' dipole strength can be related to the parameters of the symmetry energy and to the neutron skin thickness on the grounds of a relativistic quasiparticle random-phase approximation. Using this ansatz and the experimental findings for {sup 130}Sn and {sup 132}Sn, we derive a value of the symmetry energy pressure of p-bar{sub 0} = 2.2+-0.5 MeV/fm{sup 3}. Neutron skin thicknesses of R{sub n}-R{sub p} 0.23+-0.03 fm and 0.24+-0.03 fm for {sup 130}Sn and {sup 132}Sn, respectively, have been determined. Preliminary results on {sup 68}Ni from a similar experiment using an improved setup indicate an enhanced cross section at low energies, while the results for {sup 58}Ni are in accordance with results from photoabsorption measurements.
- OSTI ID:
- 21344570
- Journal Information:
- AIP Conference Proceedings, Vol. 1165, Issue 1; Conference: International conference on nuclear structure and dynamics '09, Dubrovnik (Croatia), 4-8 May 2009; Other Information: DOI: 10.1063/1.3232065; (c) 2009 American Institute of Physics; ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
Similar Records
Nuclear symmetry energy and neutron skins derived from pygmy dipole resonances
Connecting Nuclear Structure to Stellar Astrophysics: Neutron Skin in Tin Isotopes
Related Subjects
ANTIPROTONS
CROSS SECTIONS
DIPOLES
EQUATIONS OF STATE
GIANT RESONANCE
MEV RANGE
NEUTRON-RICH ISOTOPES
NEUTRONS
NICKEL 58
NICKEL 68
NUCLEAR STRUCTURE
RANDOM PHASE APPROXIMATION
RELATIVISTIC RANGE
SHELL MODELS
SKIN
STRENGTH FUNCTIONS
TIN 130
TIN 132
ANTIBARYONS
ANTIMATTER
ANTINUCLEI
ANTINUCLEONS
ANTIPARTICLES
APPROXIMATIONS
BARYONS
BETA DECAY RADIOISOTOPES
BETA-MINUS DECAY RADIOISOTOPES
BODY
CALCULATION METHODS
ELEMENTARY PARTICLES
ENERGY RANGE
EQUATIONS
EVEN-EVEN NUCLEI
FERMIONS
FUNCTIONS
HADRONS
INTERMEDIATE MASS NUCLEI
ISOTOPES
MATHEMATICAL MODELS
MATTER
MINUTES LIVING RADIOISOTOPES
MULTIPOLES
NICKEL ISOTOPES
NUCLEAR MODELS
NUCLEI
NUCLEONS
ORGANS
PROTONS
RADIOISOTOPES
RESONANCE
SECONDS LIVING RADIOISOTOPES
STABLE ISOTOPES
TIN ISOTOPES