Neutron Skin and Equation of State in Asymmetric Nuclear Matter

Details Neutron Skin and Equation of State in Asymmetric Nuclear Matter Neutron Skin and Equation of State in Asymmetric Nuclear Matter

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..557y&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

Neutron skin thickness of stable and unstable nuclei are studied by using Skyrme Hartree-Fock (SHF) models and relativistic mean field (RMF) models in relation with the pressure of EOS in neutron matter. We found a clear linear correlation between the neutron skin sizes in heavy nuclei, 132Sn and 208Pb and the pressure of neutron matter in both SHF and RMF, while the correlation is weak in unstable nuclei 32Mg and 44Ar.

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