Construct an EOS for use in astrophysics: neutron stars and supernovae wide parameter range: proton fraction Large charge asymmetry: thus investigation.
Pavel Stránský 1,2 3 rd Chaotic Modeling and Simulation International Conference, Chania, Greece, 2010 3 rd January 2010 1 Institute of Particle and Nuclear.
Construct an EOS for use in astrophysics: neutron stars and supernovae wide parameter range:
