Equation of State of Nuclear Matter, Neutron Rich Nuclei in Laboratories and Pasta Nuclei in Neutron Star Crusts(Proceedings of the YITP Workshop on Nuclear Matter under Extreme Conditions)
Macroscopic properties of neutron rich nuclei in laboratories and nuclei in neutron star crusts are supposed to be dominated by the equation of state (EOS) of asymmetric nuclear matter. In this study, we attempt to identify the most important EOS parameter that governs these properties.
Progress of theoretical physics. Supplement
[List of Volumes]
Progress of theoretical physics. Supplement (156), 137-138, 2004-12-28
[Table of Contents]
Publication Office, Progress of Theoretical Physics
You must have a user ID to see the references.If you already have a user ID, please click "Login" to access the info.New users can click "Sign Up" to register for an user ID.