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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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dc.citation.conferencePlace KO -
dc.citation.conferencePlace Seoul -
dc.citation.startPage 04011 -
dc.citation.title 13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017 -
dc.contributor.author Lee, Chang-Hwan -
dc.contributor.author Lim, Yeunhwan -
dc.contributor.author Hyun, Chang Ho -
dc.contributor.author Kwak, Kyujin -
dc.date.accessioned 2023-12-19T18:38:37Z -
dc.date.available 2023-12-19T18:38:37Z -
dc.date.created 2018-03-12 -
dc.date.issued 2017-07-03 -
dc.description.abstract Neutron star provides unique environments for the investigation of the physics of extreme dense matter beyond normal nuclear saturation density. In such high density environments, hadrons with strange quarks are expected to play very important role in stabilizing the system. Kaons and hyperons are the lowest mass states with strangeness among meson and bayron families, respectively. In this work, we investigate the role of kaons and hyperons to the neutron star mass, and discuss their role in the neutron star cooling -
dc.identifier.bibliographicCitation 13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017, pp.04011 -
dc.identifier.doi 10.1051/epjconf/201816804011 -
dc.identifier.issn 2101-6275 -
dc.identifier.scopusid 2-s2.0-85040985943 -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/35285 -
dc.identifier.url https://www.epj-conferences.org/10.1051/epjconf/201816804011 -
dc.language 영어 -
dc.publisher 13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017 -
dc.title Role of strangeness to the neutron star mass and cooling -
dc.type Conference Paper -
dc.date.conferenceDate 2017-07-03 -

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