Nuclear matter symmetry energy and the neutron skin thickness of heavy nuclei

Lie-Wen Chen, Che Ming Ko, and Bao-An Li
Phys. Rev. C 72, 064309 – Published 15 December 2005

Abstract

Correlations between the thickness of the neutron skin in finite nuclei and the nuclear matter symmetry energy are studied in the Skyrme Hartree-Fock model. From the most recent analysis of the isospin diffusion data in heavy-ion collisions based on an isospin- and momentum-dependent transport model with in-medium nucleon-nucleon cross sections, a value of L=88±25 MeV for the slope of the nuclear symmetry energy at saturation density is extracted, and this imposes stringent constraints on both the parameters in the Skyrme effective interactions and the neutron skin thickness of heavy nuclei. Predicted thickness of the neutron skin is 0.22±0.04 fm for Pb208, 0.29±0.04 fm for Sn132, and 0.22±0.04 fm for Sn124.

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  • Received 5 September 2005

DOI:https://doi.org/10.1103/PhysRevC.72.064309

©2005 American Physical Society

Authors & Affiliations

Lie-Wen Chen1,2, Che Ming Ko3, and Bao-An Li4

  • 1Institute of Theoretical Physics, Shanghai Jiao Tong University, Shanghai 200240, China
  • 2Center of Theoretical Nuclear Physics, National Laboratory of Heavy Ion Accelerator, Lanzhou 730000, China
  • 3Cyclotron Institute and Physics Department, Texas A&M University, College Station, Texas 77843-3366
  • 4Department of Chemistry and Physics, P.O. Box 419, Arkansas State University, State University, Arkansas 72467-0419

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Issue

Vol. 72, Iss. 6 — December 2005

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