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Many-body theory of nuclear and neutron star matter

V. R. Pandharipande·A. Akmal·D. G. Ravenhall
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Abstract

We present results obtained for nuclei, nuclear and neutron star matter, and neutron star structure obtained with the recent Argonne v18 two- nucleon and Urbana IX three-nucleon interactions including relativistic boost corrections. These interactions predict that matter will undergo a transition to a spin layered phase with neutral pion condensation. We also consider the possibility of a transition to quark matter.

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V. R. Pandharipande, A. Akmal, D. G. Ravenhall. 1998-02-16. Many-body theory of nuclear and neutron star matter. https://arxiv.org/abs/nucl-th/9802048

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