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Symmetry energy within the BHF approach

Rios Huguet, A, Vidana, I, Polls, A and Providencia, C (2012) Symmetry energy within the BHF approach Journal of Physics: Conference Series, 342, 012012.

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Abstract

We analyze the correlations of the slope and curvature parameters of the symmetry energy with the neutron skin thickness of neutron-rich isotopes, and the crust-core transition density in neutron stars. Microscopic Brueckner–Hartree–Fock results are compared with those obtained with several Skyrme and relativistic mean field models. Our results confirm that there is an inverse correlation between the neutron skin thickness and the transition density.

Item Type: Article
Divisions : Faculty of Engineering and Physical Sciences > Physics
Authors :
AuthorsEmailORCID
Rios Huguet, AUNSPECIFIEDUNSPECIFIED
Vidana, IUNSPECIFIEDUNSPECIFIED
Polls, AUNSPECIFIEDUNSPECIFIED
Providencia, CUNSPECIFIEDUNSPECIFIED
Date : 1 October 2012
Identification Number : 10.1088/1742-6596/342/1/012012
Additional Information : Copyright 2012 Institute of Physics. This is the author's accepted manuscript.
Depositing User : Symplectic Elements
Date Deposited : 08 Mar 2013 12:30
Last Modified : 23 Sep 2013 20:01
URI: http://epubs.surrey.ac.uk/id/eprint/758756

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