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Article: Does kaon condensation occur in neutron stars in the relativistic mean-field theory?

TitleDoes kaon condensation occur in neutron stars in the relativistic mean-field theory?
Authors
Issue Date1997
PublisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/physletb
Citation
Physics Letters, Section B: Nuclear, Elementary Particle And High-Energy Physics, 1997, v. 401 n. 3-4, p. 219-223 How to Cite?
AbstractWe discuss whether kaon condensation occurs in neutron star matter by using the Zimanyi-Moszkowski model in the relativistic mean-field theory. As a comparison, we also discuss the results from the Boguta-Bodmer model. We show that even though hyperons which may increase the critical condensation density are not included, kaon condensation might not occur in stable neutron stars for the Zimanyi-Moszkowski model. © 1997 Elsevier Science B.V.
Persistent Identifierhttp://hdl.handle.net/10722/174870
ISSN
2015 Impact Factor: 4.787
2015 SCImago Journal Rankings: 3.186
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorDai, ZGen_US
dc.contributor.authorCheng, KSen_US
dc.date.accessioned2012-11-26T08:47:54Z-
dc.date.available2012-11-26T08:47:54Z-
dc.date.issued1997en_US
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle And High-Energy Physics, 1997, v. 401 n. 3-4, p. 219-223en_US
dc.identifier.issn0370-2693en_US
dc.identifier.urihttp://hdl.handle.net/10722/174870-
dc.description.abstractWe discuss whether kaon condensation occurs in neutron star matter by using the Zimanyi-Moszkowski model in the relativistic mean-field theory. As a comparison, we also discuss the results from the Boguta-Bodmer model. We show that even though hyperons which may increase the critical condensation density are not included, kaon condensation might not occur in stable neutron stars for the Zimanyi-Moszkowski model. © 1997 Elsevier Science B.V.en_US
dc.languageengen_US
dc.publisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/physletben_US
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physicsen_US
dc.rightsPhysics Letters Section B: Nuclear, Elementary Particle and High-Energy Physics. Copyright © Elsevier BV.-
dc.titleDoes kaon condensation occur in neutron stars in the relativistic mean-field theory?en_US
dc.typeArticleen_US
dc.identifier.emailCheng, KS: hrspksc@hkucc.hku.hken_US
dc.identifier.authorityCheng, KS=rp00675en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1016/S0370-2693(97)00416-4-
dc.identifier.scopuseid_2-s2.0-0042762932en_US
dc.identifier.hkuros25843-
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0042762932&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume401en_US
dc.identifier.issue3-4en_US
dc.identifier.spage219en_US
dc.identifier.epage223en_US
dc.identifier.isiWOS:A1997XC55000003-
dc.publisher.placeNetherlandsen_US
dc.identifier.scopusauthoridDai, ZG=7201387760en_US
dc.identifier.scopusauthoridCheng, KS=9745798500en_US

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