Effects of strong magnetic fields in dense stellar matter

被引：0
|
作者：
Lavagno, A. [1 ]
Lingua, F.
机构：
[1] Politecn Torino, Dept Appl Sci & Technol, I-10129 Turin, Italy
来源：
MAGNETIC FIELDS THROUGHOUT STELLAR EVOLUTION | 2014年 / 302期
关键词：
Relativistic equation of state; Delta baryonic resonances; Compact stars;
D O I：
10.1017/S1743921314002695
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We study the effects of strong magnetic fields in dense stellar matter within an effective relativistic equation of state with the inclusion of hyperons and Delta(1232)-isobar degrees of freedom. The effects of high magnetic field interactions significantly affect the nuclear equation of state and the macroscopic properties of the star. In this framework we investigate the role of the presence of the Delta-isobars degrees of freedom in structure and in the bulk properties of the compact star.
引用
收藏
页码：439 / 440
页数：2
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