Kaon condensation in neutron star using relativistic mean field models

被引：0

作者：

Hong, S. W. ^{[1
]}

Hyun, C. H. ^{[1
]}

Ryu, C. Y. ^{[2
]}

机构：

[1] Sungkyunkwan Univ, Dept Phys, Suwon 440746, South Korea

[2] RCNP, Ibaraki 5670047, Japan

来源：

PROCEEDINGS OF THE IX INTERNATIONAL CONFERENCE ON HYPERNUCLEAR AND STRANGE PARTICLE PHYSICS | 2007年

关键词：

D O I：

10.1007/978-3-540-76367-3_79

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We use the modified quark-meson coupling and the quantum hadrodynamics models to study the properties of neutron star. Coupling constants of both models are adjusted to reproduce the same saturation properties. The onset of kaon condensation in neutron star matter is studied in detail over a wide range of kaon optical potential values. Once the kaon condensation takes place, the population of kaons increases very rapidly, and kaons become the dominant component, possibly making the neutron star matter a kaonic matter if the kaon optical potential is large.

引用

页码：393 / +

页数：2

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