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Nuclear Equation of State and Neutron Star Structure

A. E. L. Dieperink·D. Van Neck·Y. Dewulf·V. Rodin
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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 from the neutron skin of finite nuclei are considered.

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A. E. L. Dieperink, D. Van Neck, Y. Dewulf, V. Rodin. 2003-12-03. Nuclear Equation of State and Neutron Star Structure. https://arxiv.org/abs/nucl-th/0312012

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