Structure of the pygmy dipole resonance in 124Sn

J. Endres, D. Savran, P. A. Butler, M. N. Harakeh, S. Harissopulos, R. -D. Herzberg, R Krucken, A. Lagoyannis, E. Litvinova, N. Pietralla, V. Yu. Ponomarev, L. Popescu, P. Ring, M. Scheck, F Schluter, K. Sonnabend, V. I. Stoica, H. J. Wortche, A. Zilges

Research output: Contribution to journalArticle

Abstract

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 124Sn by means of the (α,α′γ) coincidence method at Eα=136MeV 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 124Sn by comparing the differential cross sections measured in (α,α′γ) to results stemming from (γ,γ′) 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 (γ,γ′) 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.
Original languageEnglish
Article number064331
JournalPhysical Review C
Volume85
Issue number6
DOIs
Publication statusPublished - 28 Jun 2012
Externally publishedYes

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dipoles
electric dipoles
nuclei
neutrons
oscillations
Netherlands
nuclear structure
astrophysics
signatures
spectrometers
thresholds
energy
cross sections
photons
approximation
scattering

Cite this

Endres, J., Savran, D., Butler, P. A., Harakeh, M. N., Harissopulos, S., Herzberg, R. -D., ... Zilges, A. (2012). Structure of the pygmy dipole resonance in 124Sn. Physical Review C, 85(6), [064331]. https://doi.org/10.1103/PhysRevC.85.064331
Endres, J. ; Savran, D. ; Butler, P. A. ; Harakeh, M. N. ; Harissopulos, S. ; Herzberg, R. -D. ; Krucken, R ; Lagoyannis, A. ; Litvinova, E. ; Pietralla, N. ; Ponomarev, V. Yu. ; Popescu, L. ; Ring, P. ; Scheck, M. ; Schluter, F ; Sonnabend, K. ; Stoica, V. I. ; Wortche, H. J. ; Zilges, A. / Structure of the pygmy dipole resonance in 124Sn. In: Physical Review C. 2012 ; Vol. 85, No. 6.
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abstract = "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 124Sn by means of the (α,α′γ) coincidence method at Eα=136MeV 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 124Sn by comparing the differential cross sections measured in (α,α′γ) to results stemming from (γ,γ′) 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 (γ,γ′) 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.",
author = "J. Endres and D. Savran and Butler, {P. A.} and Harakeh, {M. N.} and S. Harissopulos and Herzberg, {R. -D.} and R Krucken and A. Lagoyannis and E. Litvinova and N. Pietralla and Ponomarev, {V. Yu.} and L. Popescu and P. Ring and M. Scheck and F Schluter and K. Sonnabend and Stoica, {V. I.} and Wortche, {H. J.} and A. Zilges",
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Endres, J, Savran, D, Butler, PA, Harakeh, MN, Harissopulos, S, Herzberg, R-D, Krucken, R, Lagoyannis, A, Litvinova, E, Pietralla, N, Ponomarev, VY, Popescu, L, Ring, P, Scheck, M, Schluter, F, Sonnabend, K, Stoica, VI, Wortche, HJ & Zilges, A 2012, 'Structure of the pygmy dipole resonance in 124Sn' Physical Review C, vol. 85, no. 6, 064331. https://doi.org/10.1103/PhysRevC.85.064331

Structure of the pygmy dipole resonance in 124Sn. / Endres, J.; Savran, D.; Butler, P. A.; Harakeh, M. N.; Harissopulos, S.; Herzberg, R. -D.; Krucken, R ; Lagoyannis, A.; Litvinova, E.; Pietralla, N.; Ponomarev, V. Yu.; Popescu, L.; Ring, P.; Scheck, M.; Schluter, F ; Sonnabend, K.; Stoica, V. I.; Wortche, H. J.; Zilges, A.

In: Physical Review C, Vol. 85, No. 6, 064331, 28.06.2012.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Structure of the pygmy dipole resonance in 124Sn

AU - Endres, J.

AU - Savran, D.

AU - Butler, P. A.

AU - Harakeh, M. N.

AU - Harissopulos, S.

AU - Herzberg, R. -D.

AU - Krucken, R

AU - Lagoyannis, A.

AU - Litvinova, E.

AU - Pietralla, N.

AU - Ponomarev, V. Yu.

AU - Popescu, L.

AU - Ring, P.

AU - Scheck, M.

AU - Schluter, F

AU - Sonnabend, K.

AU - Stoica, V. I.

AU - Wortche, H. J.

AU - Zilges, A.

PY - 2012/6/28

Y1 - 2012/6/28

N2 - 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 124Sn by means of the (α,α′γ) coincidence method at Eα=136MeV 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 124Sn by comparing the differential cross sections measured in (α,α′γ) to results stemming from (γ,γ′) 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 (γ,γ′) 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.

AB - 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 124Sn by means of the (α,α′γ) coincidence method at Eα=136MeV 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 124Sn by comparing the differential cross sections measured in (α,α′γ) to results stemming from (γ,γ′) 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 (γ,γ′) 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.

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DO - 10.1103/PhysRevC.85.064331

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VL - 85

JO - Physical Review C

JF - Physical Review C

SN - 2469-9985

IS - 6

M1 - 064331

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Endres J, Savran D, Butler PA, Harakeh MN, Harissopulos S, Herzberg R-D et al. Structure of the pygmy dipole resonance in 124Sn. Physical Review C. 2012 Jun 28;85(6). 064331. https://doi.org/10.1103/PhysRevC.85.064331