Coupling of nuclear and electron modes in relativistic stellar matter

Details Coupling of nuclear and electron modes in relativistic stellar matter Coupling of nuclear and electron modes in relativistic stellar matter

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvc..74d5802p&link_type=abstract

Physical Review C, vol. 74, Issue 4, id. 045802

Physics

11

Nuclear Matter Aspects Of Neutron Stars, Nuclear Structure Models And Methods, Nuclear Matter, Relativistic Models

Scientific paper

The conditions under which nuclear collective modes couple to plasmon modes in asymmetric nuclear matter (ANM) neutralized by electrons, which is of interest for the study of neutron stars and supernovae, are investigated. The calculations were performed within a relativistic mean-field approach to nuclear matter, and the Coulomb field was included. We show that the coupling may be so strong that it affects the onset of the nuclear mode at low densities and may also affect its isovector/isoscalar character.

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