Many-body theory of nuclear and neutron star matter

Details Many-body theory of nuclear and neutron star matter Many-body theory of nuclear and neutron star matter

1998-02-16

arxiv.org/abs/nucl-th/9802048v1

Physics

Nuclear Physics

Nuclear Theory

18 pages, 10 figures included as .eps files. To appear in "Hirschegg '98: Nuclear Astrophysics", Proc. Int. Workshop XXVI on G

Scientific paper

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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