The Equation of State for Baryonic Matter

Physics – Nuclear Physics – Nuclear Theory

Scientific paper

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Scientific paper

The current status of the Equation of State (EOS) used in strongly interacting matter and models of the supernova phenomenon and neutron stars is reviewed. The key role of understanding the nucleon-nucleon interaction and interactions in exotic matter (strange baryons, meson condensates and deconfined quarks) is emphasised. A brief survey of experimental and observational quantities which may help to characterize these interactions is given. Example of such characterization is given for the phenomenological Skyrme interaction. Preliminary results for the EOS based on a nucleon-nucleon interaction derived from a non-relativistic one-gluon-exchange-quark model are shown for pure neutron and symmetric nuclear matter.

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