Kaon condensation and lambda-nucleon loop in the relativistic mean-field approach

dc.contributor.authorMaruyama T.
dc.contributor.authorMuto T.
dc.contributor.authorTatsumi T.
dc.contributor.authorTsushima K.
dc.contributor.authorThomas A.W.
dc.date.accessioned2024-03-13T01:43:44Z
dc.date.available2024-03-13T01:43:44Z
dc.date.issued2005
dc.description.abstractThe 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 K̄s state carrying the same quantum numbers as the antikaon. The appearance of the K̄s 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 K - K̄s 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 Λ-mixing effects in the ground state of high-density matter. Implications of K K̄s condensation for high-energy heavy-ion collisions are briefly mentioned. © 2005 Elsevier B.V. All rights reserved.
dc.description.firstpage319
dc.description.issuenumber3-4
dc.description.lastpage345
dc.description.volume760
dc.identifier.doi10.1016/j.nuclphysa.2005.06.008
dc.identifier.issn0375-9474
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/37858
dc.relation.ispartofNuclear Physics A
dc.rightsAcesso Restrito
dc.titleKaon condensation and lambda-nucleon loop in the relativistic mean-field approach
dc.typeArtigo
local.scopus.citations17
local.scopus.eid2-s2.0-24644467714
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=24644467714&origin=inward
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