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Constraints on the symmetry energy and neutron skins from pygmy resonances in Ni68 and Sn132

Andrea Carbone, Gianluca Colò, Angela Bracco, Li-Gang Cao, Pier Francesco Bortignon, Franco Camera, and Oliver Wieland
Phys. Rev. C 81, 041301(R) – Published 2 April 2010

Abstract

Correlations between the behavior of the nuclear symmetry energy, the neutron skins, and the percentage of energy-weighted sum rule (EWSR) exhausted by the pygmy dipole resonance (PDR) in Ni68 and Sn132 are investigated by using different random phase approximation (RPA) models for the dipole response, based on a representative set of Skyrme effective forces plus meson-exchange effective Lagrangians. A comparison with the experimental data has allowed us to constrain the value of the derivative of the symmetry energy at saturation. The neutron skin radius is deduced under this constraint.

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  • Received 6 November 2009

DOI:https://doi.org/10.1103/PhysRevC.81.041301

©2010 American Physical Society

Authors & Affiliations

Andrea Carbone1, Gianluca Colò1,2, Angela Bracco1,2, Li-Gang Cao1,2,3,4, Pier Francesco Bortignon1,2, Franco Camera1,2, and Oliver Wieland2

  • 1Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy
  • 2INFN, Sezione di Milano, via Celoria 16, I-20133 Milano, Italy
  • 3Institute of Modern Physics, Chinese Academy of Science, Lanzhou 730000, People's Republic of China
  • 4Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator of Lanzhou, Lanzhou 730000, People's Republic of China

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Issue

Vol. 81, Iss. 4 — April 2010

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