Low-density instabilities in relativistic asymmetric matter of compact stars

Details Low-density instabilities in relativistic asymmetric matter of compact stars Low-density instabilities in relativistic asymmetric matter of compact stars

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvc..73b5805p&link_type=abstract

Physical Review C, vol. 73, Issue 2, id. 025805

Mathematics

Logic

26

Collective Models, Nuclear Matter, Relativistic Models, Fermi-Liquid Theory And Other Phenomenological Models

Scientific paper

Dynamical instability modes of low-density asymmetric nuclear matter (ANM) neutralized 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. The dynamical and thermodynamical instability zones are compared. It is shown that the Coulomb field quenches large structure formation but has little effect on medium and small-size fluctuations that are, however, partially stabilized by the finite range of the nuclear forces. The electron dynamics tends to restore the large-wavelength instabilities but is moderated by the high-electron Fermi energy.

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