Other
Scientific paper
Jul 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1140...69p&link_type=abstract
PROCEEDINGS OF THE NATIONAL SOCIETY OF BLACK PHYSICISTS: 35th Annual Day of Scientific Lectures & 31st Annual Meeting, 2008 Join
Other
Baryons, Neutron Stars, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Phase Transitions: General Studies, Electron States At Surfaces And Interfaces
Scientific paper
Understanding the equation of state (EOS) of cold nuclear matter, namely, the relation between pressure and energy density, is a central goal of nuclear physics that cuts across a variety of disciplines. Indeed, the limits of nuclear existence, the collision of heavy ions, the structure of neutron stars, and the dynamics of core-collapse supernova, all depend critically on the equation of state of hadronic matter. In this contribution I will concentrate on the EOS of cold baryonic matter with special emphasis on its impact on the structure and dynamics of neutron stars. In particular, I will discuss the many fascinating phases that one encounters in the journey from the low-density crust to the high-density core.
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