Kaon Condensation and Lambda-Nucleon Loop in the Relativistic Mean-Field Approach
arXiv:nucl-th/0502079 · doi:10.1016/j.nuclphysa.2005.06.008
Abstract
The possibility of kaon condensation in high-density symmetric nuclear matter is investigated including both s- and p-wave kaon-baryon interactions within the relativistic mean-field (RMF) theory. Above a certain density, we have a collective state carrying the same quantum numbers as the antikaon. The appearance of the state is caused by the time component of the axial-vector interaction between kaons and baryons. It is shown that the system becomes unstable with respect to condensation of - pairs. We consider how the effective baryon masses affect the kaon self-energy coming from the time component of the axial-vector interaction. Also, the role of the spatial component of the axial-vector interaction on the possible existence of the collective kaonic states is discussed in connection with -mixing effects in the ground state of high-density matter. Implications of condensation for high-energy heavy-ion collisions are briefly mentioned.
27 pages text, 8 figures
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- The Role of Baryon Structure in Neutron Stars
- The effect of Kaon Condensation on Quark-Antiquark Condensate in Dense Matter
- Pseudoscalar mesons from a PNJL model at zero temperature