Kaon Condensation in Dense Stellar Matter
arXiv:hep-ph/9503382 · doi:10.1016/0370-1573(96)00005-1
Abstract
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 $2\lsim ρ/ρ_0\lsim 4$, in the range to allow the intriguing new phenomena predicted by Brown and Bethe to take place in compact star matter.
29 pages, epsfig.sty, 7 figure(uuencoded)
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- Deeply-bound state in the He(in-flight , ) spectrum and its moving pole near the threshold
- Thermal and Quantum Fluctuations in the Kaon Condensed Phase
- Protoneutron Stars with Kaon Condensation and their Delayed Collapse
- K^+ production in baryon-baryon and heavy-ion collisions
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