Low-Density Instabilities in Relativistic Hadronic Models

Details Low-Density Instabilities in Relativistic Hadronic Models Low-Density Instabilities in Relativistic Hadronic Models

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008esnm.conf..126p&link_type=abstract

EXOTIC STATES OF NUCLEAR MATTER. Proceedings of the International Symposium EXOCT07. Held 11-15 June 2007 in Catania University,

Computer Science

Asymmetric Nuclear Matter, Stellar Matter, Distillation Effect

Scientific paper

Dynamical instability modes and thermodynamical instabilities of low-density asymmetric nuclear matter (ANM) neutralised by electrons as found in supernova core and neutron star crust are studied in the framework of relativistic mean-field hadron models with the inclusion of electron and photon fields. Both models with constant and density dependent coupling constants are considered. It is shown that the Coulomb field quenches large structure formation but has little effect on medium and small-size fluctuations. Implications on the crust of compact stars are discussed.

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