arXiv:nucl-th/9802048·v1·Nuclear Theory
Many-body theory of nuclear and neutron star matter
V.R. Pandharipande🇺🇸 · A. Akmal🇺🇸 · D.G. Ravenhall🇺🇸
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.
Comments: 18 pages, 10 figures included as .eps files. To appear in "Hirschegg '98: Nuclear Astrophysics", Proc. Int. Workshop XXVI on Gross Properties of Nuclei and Nuclear Excitations, January 11-17, 1998, Hirschegg, Austria