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Structure of the pygmy dipole resonance in 124 Sn

2012; American Institute of Physics; Volume: 85; Issue: 6 Linguagem: Inglês

10.1103/physrevc.85.064331

1538-4497

J. Endres, D. Savran, P. A. Butler, M.N. Harakeh, S. Harissopulos, R.‐D. Herzberg, R. Krücken, A. Lagoyannis, Елена Литвинова, N. Pietralla, V. Yu. Ponomarev, L. Popescu, P. Ring, M. Scheck, Felix Schlüter, K. Sonnabend, Victor Stoica, H. J. Wörtche, A. Zilges,

Astronomical and nuclear sciences

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 ${}^{124}$Sn by means of the $(\ensuremath{\alpha},{\ensuremath{\alpha}}^{\ensuremath{'}}\ensuremath{\gamma})$ coincidence method at ${E}_{\ensuremath{\alpha}}=136\phantom{\rule{0.28em}{0ex}}\mathrm{MeV}$ 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 ${}^{124}$Sn by comparing the differential cross sections measured in $(\ensuremath{\alpha},{\ensuremath{\alpha}}^{\ensuremath{'}}\ensuremath{\gamma})$ to results stemming from $(\ensuremath{\gamma},{\ensuremath{\gamma}}^{\ensuremath{'}})$ 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 $(\ensuremath{\gamma},{\ensuremath{\gamma}}^{\ensuremath{'}})$ 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.