Many-body Theory of Nuclear and Neutron Star Matter
نویسندگان
چکیده
We present results obtained for nuclei, nuclear and neutron star matter, and neutron star structure obtained with the recent Argonne v18 twonucleon 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.
منابع مشابه
Microscopic many-body theory of nuclei and neutron star matter
We review the recent progress in application of microscopic many-body theory, based on realistic twoand threenucleon interactions, to nuclei and neutron star matter. Modern models of nuclear interactions are discussed along with quantum Monte Carlo methods used to calculate nuclear and nucleon matter properties. Essentially exact Green’s function Monte Carlo calculations have been successfully ...
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تاریخ انتشار 1998