Nucleosynthesis in Advection-Dominated Accretion Flow onto a Black Hole

被引：1

作者：

Zhang, Jiang ^{[1
,2
]}

Ma, Ren-Yi ^{[3
]}

Li, Hong-Jie ^{[4
]}

Zhang, Bo ^{[5
]}

机构：

[1] Hebei GEO Univ, Dept Math & Sci, Shijiazhuang 050016, Peoples R China

[2] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China

[3] Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China

[4] Hebei Univ Sci & Technol, Sch Sci, Shijiazhuang 050016, Peoples R China

[5] Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Peoples R China

来源：

CHINESE PHYSICS LETTERS | 2017年 / 34卷 / 04期

基金：

中国国家自然科学基金;

关键词：

STELLAR HYDRODYNAMICS; DISKS;

D O I：

10.1088/0256-307X/34/4/049701

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Nucleosynthesis in advection-dominated accretion flow (ADAF) onto a black hole is proposed to be an important role in chemical evolution around compact stars. We investigate the nucleosynthesis in ADAF relevant for a black hole of low mass, different from that of the self-similar solution. In particular, the presence of supersolar metal mass fractions of some isotopes seems to be associated with the known black hole nucleosynthesis in ADAF, which offers further evidence of diversity of the chemical enrichment.

引用

页数：4

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