Kaon condensation in the quark-meson coupling model and compact stars -: art. no. 035802

被引：60
作者：
Menezes, DP
Panda, PK
Providência, C
机构：
[1] Univ Fed Santa Catarina, Ctr Ciencias Fis & Matemat, Dept Fis, BR-88040900 Florianopolis, SC, Brazil
[2] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
[3] Univ Coimbra, Dept Fis, Ctr Fis Teor, P-3004516 Coimbra, Portugal
来源：
PHYSICAL REVIEW C | 2005年 / 72卷 / 03期
关键词：
D O I：
10.1103/PhysRevC.72.035802
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
The properties of neutron stars, consisting of a crust of hadrons and an internal part of hadrons and kaon condensate, are calculated within the quark-meson-coupling model. We considered stars with nucleons only in the hadron phase and also stars with hyperons as well. The results are compared with the ones obtained from the nonlinear Walecka model for the hadronic phase.
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页数：7
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