Nuclear Equation of State and Neutron Star Structure

Details Nuclear Equation of State and Neutron Star Structure Nuclear Equation of State and Neutron Star Structure

2003-12-03

arxiv.org/abs/nucl-th/0312012v1

Physics

Nuclear Physics

Nuclear Theory

Invited talk presented at the Advanced Research Workshop on "Superdense QCD Matter and Compact Stars", Yerevan, Armenia, Sep 2

Scientific paper

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 from the neutron skin of finite nuclei are considered.

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