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dc.contributor.author노만규-
dc.date.accessioned2018-02-22T04:13:12Z-
dc.date.available2018-02-22T04:13:12Z-
dc.date.issued2012-02-
dc.identifier.citationInternational Journal of Mordern Physics Conference, 2012, P.123-130en_US
dc.identifier.issn2010-1945-
dc.identifier.urihttps://arxiv.org/abs/1202.2645?-
dc.identifier.urihttps://www.worldscientific.com/doi/abs/10.1142/S2010194512005831-
dc.description.abstractWe explore the possibility of three phases in the core of neutron star in a form of triple layers. From the center, strange quark matter, kaon condensed nuclear matter and nuclear matter form a triple layer. We discuss how the phase of strange quark matter is smoothly connected to kaon condensed nuclear matter phase. We also demonstrate that the compact star with triple layered structure can be a model compatible with the 1.97-solar-mass object PSR J1614-2230 recently observed.Comment: 8 pages, 2 figures, to appear in the Proceedings of the Symposium on Cosmology and Particle Astrophysics (CosPA2011), October 28-31, 2011, Beijing, Chinaen_US
dc.language.isoenen_US
dc.publisherWorld Scientific Publishing Companyen_US
dc.titleTriple layered compact star with strange quark matteren_US
dc.typeArticleen_US
dc.relation.no01-
dc.relation.volume10-
dc.identifier.doi10.1142/S2010194512005831-
dc.relation.page123-130-
dc.contributor.googleauthorKim, Kyungmin-
dc.contributor.googleauthorLee, Hyun Kyu-
dc.contributor.googleauthorRho, Mannque-
dc.contributor.googleauthor김경민-
dc.contributor.googleauthor이현규-
dc.contributor.googleauthor노만규-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidrho-
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COLLEGE OF NATURAL SCIENCES[S](자연과학대학) > PHYSICS(물리학과) > Articles
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