Surface structure of quark stars with magnetic fields

被引：1
|
作者：
Jaikumar, Prashanth [1 ]
机构：
[1] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA
来源：
PRAMANA-JOURNAL OF PHYSICS | 2006年 / 67卷 / 05期
关键词：
quark stars; magnetic fields; nucleosynthesis; STRANGE; TEMPERATURE; EMISSION; MATTER;
D O I：
10.1007/s12043-006-0104-z
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We investigate the impact of magnetic fields on the electron distribution of the electrosphere of quark stars. For moderately strong magnetic fields of B similar to 10(13) G, quantization effects are generally weak due to the large number density of electrons at surface, but can nevertheless affect the photon emission properties of quark stars. We outline the main observational characteristics of quark stars as determined by their surface emission, and briefly discuss their formation in explosive events termed as quark-novae, which may be connected to the r-process.
引用
收藏
页码：937 / 949
页数：13
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