Kaon condensation in hyperonic matter and structure of neutron stars

被引：0

作者：

Muto, T ^{[1
]}

机构：

[1] Chiba Inst Technol, Dept Phys, Narashino, Chiba 2750023, Japan

来源：

PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT | 2004年 / 156期

关键词：

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The effects of kaon condensates on the equation of state (EOS) in hyperonic matter, where hyperons (A, Sigma(-)) are mixed in the ground state of neutron-star matter, are investigated. In the fully-developed phase of kaon condensation, it is shown that the EOS is much softened due to the s-wave kaon-baryon interactions as well as due to the hyperon-mixing. As a result, the energy of the system has a local minimum, which leads to a metastable self-bound kaon-condensed star in addition to a kaon-condensed star obtained by Maxwell's construction. The lifetime of the metastable state of the kaon-condensed bound star is estimated.

引用

页码：182 / 183

页数：2

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