Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sqm..conf..283l&link_type=abstract
International Symposium on Strangeness and Quark Matter, p. 283 - 297
Astronomy and Astrophysics
Astrophysics
Baryons, Equations Of State, Interstellar Matter, Kaons, Mesons, Neutron Stars, Perturbation Theory, Elementary Particle Interactions, Formalism, Nucleons, Solitary Waves, Symmetry
Scientific paper
This article combines two talks given by the authors and is based on works done in collaboration with G.E. Brown and D.P. Min on kaon condensation in dense baryonic medium treated in chiral perturbation theory using heavy-baryon formalism. It contains, in addition to what was recently published, astrophysical backgrounds for kaon condensation discussed by Brown and Bethe, a discussion on a renormalization-group analysis to meson condensation worked out together with H.K. Lee and S.J. Sin, and the recent results of K.M. Westerberg in the bound-state approach to the Skyrme model. Negatively charged kaons are predicted to condense at a critical density 2 approx. less than rho/rhoo approx. less than 4, in the range to allow the intriguing new phenomena predicted by Brown and Bethe to take place in compact star matter.
Lee Chang-Hwan
Rho Mannque
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