Multi-Antikaonic Nuclei and Kaon Condensation in Dense Matter

Details Multi-Antikaonic Nuclei and Kaon Condensation in Dense Matter Multi-Antikaonic Nuclei and Kaon Condensation in Dense Matter

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..233m&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Physics

Kaon-Kaon Interactions, Neutron Stars, Chiral Symmetries, Meson-Nucleon Interactions, Electric Potential, Kaon-Induced Reactions, Neutron Stars, Chiral Symmetries, Coulomb Energies

Scientific paper

The structure of multi-antikaonic nuclei (MKN) is investigated in a relativistic mean-field theory coupled with the nonlinear K- field by the use of effective chiral Lagrangian. The effects of the Λ(1405) range terms on the structure of the MKN are taken into account. It is shown that baryon number density exceeds three times the normal saturation density in the central region of the MKN that a neutron skin structure becomes remarkable as the number of the embedded K- mesons increases. The similarity difference between the MKN kaon condensation in neutron stars are discussed.

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