CONSTRAINTS ON THE EQUATION OF STATE FROM NEUTRON-STARS AND HYBRID STARS

被引：3

作者：

ROSENHAUER, A

STAUBO, EF

CSERNAI, LP

机构：

[1] Department of Physics, University of Bergen, Bergen

来源：

ZEITSCHRIFT FUR PHYSIK A-HADRONS AND NUCLEI | 1992年 / 342卷 / 02期

关键词：

D O I：

10.1007/BF01288475

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：

Hybrid stars composed of a strange matter core surrounded by neutron matter are investigated. We apply star models based on phenomenological equations of state (EOS) from nuclear reactions including a phase transition between the hadronic phase and the quark gluon plasma. For specific equations of state hybrid stars might exist. While the nuclear part of the EOS has only a minor influence on the properties of hybrid stars, the EOS for the quark gluon phase has a crucial impact on the existence of such objects.

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页码：235 / 238

页数：4

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