Kaon Condensation in Dense Stellar Matter

Details Kaon Condensation in Dense Stellar Matter Kaon Condensation in Dense Stellar Matter

1994-11-23

arxiv.org/abs/hep-ph/9411364v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, epsfig.sty, 1 figure(uuencoded)

Scientific paper

This talk is based on work 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, some new results based on the analysis on kaonic atoms by Friedman, Gal and Batty and a discussion on a renormalization-group analysis to meson condensation made together with H.K. Lee and Sin. Negatively charged kaons are predicted to condense at the critical density $2\lsim \rho/\rho_0\lsim 4$, in the range to allow all the intriguing new phenomena predicted by Brown and Bethe to take place in compact star matter.

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