中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
ELECTRON HEATING AND ACCELERATION BY MAGNETIC RECONNECTION IN HOT ACCRETION FLOWS

文献类型:期刊论文

作者Ding, Jian1; Yuan, Feng1; Liang, Edison2
刊名ASTROPHYSICAL JOURNAL
出版日期2010-01-10
卷号708期号:2页码:1545-1550
关键词acceleration of particles accretion black hole physics magnetic fields accretion disks
英文摘要Both analytical and numerical works show that magnetic reconnection must occur in hot accretion flows. This process will effectively heat and accelerate electrons. In this paper, we use the numerical hybrid simulation of magnetic reconnection plus the test-electron method to investigate the electron acceleration and heating due to magnetic reconnection in hot accretion flows. We consider fiducial values of density, temperature, and magnetic parameter beta(e) (defined as the ratio of the electron pressure to the magnetic pressure) of the accretion flow as n(0) similar to 10(6) cm(-3), T(e)(0) similar to 2 x 10(9) K, and beta(e) = 1. We find that electrons are heated to a higher temperature T(e) = 5 x 10(9) K, and a fraction eta similar to 8% of electrons are accelerated into a broken power-law distribution, dN(gamma) proportional to gamma(-p), with p approximate to 1.5 and 4 below and above similar to 1 MeV, respectively. We also investigate the effect of varying beta and n(0). We find that when beta(e) is smaller or n(0) is larger, i.e., the magnetic field is stronger, T(e), eta, and p all become larger.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]SAGITTARIUS-A-ASTERISK ; PARTICLE-ACCELERATION ; BLACK-HOLE ; GALACTIC-CENTER ; CURRENT SHEETS ; HYBRID CODE ; FIELD ; EMISSION ; MODEL ; FLARE
收录类别SCI
语种英语
WOS记录号WOS:000273021000049
公开日期2011-06-29
源URL[http://119.78.226.72//handle/331011/13379]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
2.Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA
推荐引用方式
GB/T 7714
Ding, Jian,Yuan, Feng,Liang, Edison. ELECTRON HEATING AND ACCELERATION BY MAGNETIC RECONNECTION IN HOT ACCRETION FLOWS[J]. ASTROPHYSICAL JOURNAL,2010,708(2):1545-1550.
APA Ding, Jian,Yuan, Feng,&Liang, Edison.(2010).ELECTRON HEATING AND ACCELERATION BY MAGNETIC RECONNECTION IN HOT ACCRETION FLOWS.ASTROPHYSICAL JOURNAL,708(2),1545-1550.
MLA Ding, Jian,et al."ELECTRON HEATING AND ACCELERATION BY MAGNETIC RECONNECTION IN HOT ACCRETION FLOWS".ASTROPHYSICAL JOURNAL 708.2(2010):1545-1550.

入库方式: OAI收割

来源:上海天文台

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