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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Role of strangeness to the neutron star mass and cooling

Author(s)
Lee, Chang-HwanLim, YeunhwanHyun, Chang HoKwak, Kyujin
Issued Date
2017-07-03
DOI
10.1051/epjconf/201816804011
URI
https://scholarworks.unist.ac.kr/handle/201301/35285
Fulltext
https://www.epj-conferences.org/10.1051/epjconf/201816804011
Citation
13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017, pp.04011
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
Publisher
13th International Conference on Gravitation, Astrophysics, and Cosmology. ICGAC 2017 and the 15th Italian-Korean Joint Symposium on Relativistic Astrophysics, IK 2017
ISSN
2101-6275

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