2005•Unpublished venueRequires access
Nuclear equation of state and the structure of neutron stars
Ael Dieperink, Dimitri Van Neck, Y. Dewulf, N. V. Rodin, David Bernhard Blaschke, D Dedrakian
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Abstract
The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered. 1.