Structure of the pygmy dipole resonance in124Sn
| Autor: | H. J. Wörtche, R. Krücken, Andreas Zilges, Norbert Pietralla, V. Yu. Ponomarev, R-D Herzberg, Mohsen Harakeh, Peter Ring, Lucia Popescu, P. A. Butler, Sotirios Harissopulos, V. Stoica, Kerstin Sonnabend, F. Schlüter, Elena Litvinova, J. Endres, A. Lagoyannis, Deniz Savran, Marcus Scheck |
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| Rok vydání: | 2012 |
| Předmět: | |
| Zdroj: | Physical Review C. 85 |
| ISSN: | 1089-490X 0556-2813 |
| DOI: | 10.1103/physrevc.85.064331 |
| Popis: | Background: In atomic nuclei, a concentration of electric dipole strength around the particle threshold, commonly denoted as pygmy dipole resonance, may have a significant impact on nuclear structure properties and astrophysical scenarios. A clear identification of these states and the structure of this resonance is still under discussion. Purpose: We present an experimental and theoretical study of the isospin character of the pygmy dipole resonance and investigation of a splitting of the electric dipole strength previously observed in experiments on N = 82 nuclei. Method: The pygmy dipole resonance has been studied in the semi-magic Z = 50 nucleus Sn-124 by means of the (alpha, alpha'gamma) coincidence method at E-alpha = 136 MeV using the Big-Bite Spectrometer at the Kernfysisch Versneller Instituut in Groningen, The Netherlands. Results: A splitting of the low-energy part of the electric dipole strength was identified in Sn-124 by comparing the differential cross sections measured in (alpha, alpha'gamma) to results stemming from (gamma, gamma') photon-scattering experiments. While an energetically lower-lying group of states is observed in both kinds of experiments, a higher-lying group of states is only excited in the (gamma, gamma') reaction. In addition, theoretical calculations using the self-consistent relativistic quasiparticle time-blocking approximation and the quasiparticle-phonon model have been performed. Both calculations show a qualitative agreement with the experimental data and predict a low-lying isoscalar component that is dominated by neutron-skin oscillations as expected for the pygmy dipole resonance. Furthermore, the states at higher energies show a pronounced isovector component and a different radial dependence of the corresponding transition densities as expected for the tail of the giant dipole resonance. Conclusions: An experimental signature of the neutron-skin oscillation of the pygmy dipole resonance has been corroborated. The combination of the presented reactions might make it possible to identify states of this resonance. |
| Databáze: | OpenAIRE |
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