Kaon Condensation in Dense Stellar Matter
| dc.creator | Lee, Chang-Hwan | |
| dc.creator | Rho, Mannque | |
| dc.date | 1994-11-23 | |
| dc.date.accessioned | 2026-07-07T03:57:19Z | |
| dc.date.available | 2026-07-07T03:57:19Z | |
| dc.description | 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 $2\lsim ρ/ρ_0\lsim 4$, in the range to allow all the intriguing new phenomena predicted by Brown and Bethe to take place in compact star matter. | |
| dc.description | 16 pages, epsfig.sty, 1 figure(uuencoded) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9411364 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9411364 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/45370 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Nuclear Theory | |
| dc.title | Kaon Condensation in Dense Stellar Matter | |
| dc.type | text |