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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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Kaon condensation in neutron stars with Skyrme-Hartree-Fock models

Author(s)
Lim, YeunhwanKwak, KyujinHyun, Chang HoLee, Chang-Hwan
Issued Date
2014-05
DOI
10.1103/PhysRevC.89.055804
URI
https://scholarworks.unist.ac.kr/handle/201301/48704
Fulltext
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84901940354
Citation
PHYSICAL REVIEW C, v.89, no.5
Abstract
We investigate nuclear-matter equations of state in neutron stars with kaon condensation. It is generally known that the existence of kaons in neutron star makes the equation of state soft so that the maximum mass of a neutron star is not likely to be greater than 2.0M(circle dot), the maximum mass constrained by current observations. With existing Skyrme force model parameters, we calculate nuclear equations of state and check the possibility of kaon condensation in the core of neutron stars. The results show that, even with the kaon condensation, the nuclear equation of state satisfies both the maximum mass and the allowed ranges of mass and radius.
Publisher
AMER PHYSICAL SOC
ISSN
2469-9985
Keyword
NUCLEONRADIIEQUATION-OF-STATEMATTER

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