RUI: Advanced Numerical Simulations of Black Hole Accretion
RUI: Advanced Numerical Simulations of Black Hole Accretion
批准号:
1616185
负责人:
Patrick Fragile
金额:
$22.04万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2016
资助国家:
美国
项目状态:
已结题
起止时间:
2016-07-01 至 2020-09-30
中文摘要
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英文摘要
1. The force of gravity that a black hole exerts is so strong that even light cannot escape. Some black holes form when the core of a star collapses in on itself during a supernova explosion. (A supernova is an exploding star that briefly shines as brightly as the combined light of all the hundreds of billions of stars in an entire galaxy.) Supermassive black holes, with masses millions to billions of times larger than the Sun's may lurk in the centers of most galaxies. A black hole exerts strong tidal forces that can rip apart stars that orbit it too closely. A black hole does not emit radiation itself, but the disruption of a star and infall of the resulting debris both generate considerable energy. Many accreting black hole systems exhibit rapid quasi-periodic oscillations (QPOs). Some produce jets of very high-energy plasma that speed away at velocities close to that of light. The Principal Investigator will use his improved numerical code Cosmos++ to perform simulations of accretion onto black holes. The Intellectual Merit of the proposed research is that it will advance scientists' understanding of black-hole accretion and of the nature of QPOs and properties of jets in such systems. The Broader Impacts include the involvement of students in the research project, as well as the Principal Investigator's participation in various public outreach activities and from the incorporation of his results into classroom lessons.2. The proposed research will employ the general relativistic magnetohydrodynamics (GRMHD) code Cosmos++ to perform cutting-edge simulations of black hole accretion. The Intellectual Merit of the work is that it will advance astrophysicists' understanding of the differences between viscous and MHD treatments of accretion disks around black holes, of the nature of quasi-periodic oscillations (QPOs) observed in some such systems, and of the orientation of jets in misaligned accretion systems. The Broader Impacts result from the Principal Investigator?s involvement of students in this RUI project, through a variety of public outreach activities, and from the incorporation of his results into his classroom lessons.
期刊论文(1)
专著(0)
科研奖励(0)
会议论文
On the decay of strong magnetization in global disc simulations with toroidal fields
关于环形场全局圆盘模拟中强磁化强度的衰减
DOI:
10.1093/mnras/stx274
发表时间:
2017
期刊:
Monthly Notices of the Royal Astronomical Society
影响因子:
4.8
作者:
[Fragile, P. Chris, Sądowski, Aleksander]
通讯作者:
Sądowski, Aleksander
RUI: Understanding Black Hole Accretion Across a Range of Luminosities
-
批准号:1907850
-
项目类别:Standard Grant
-
资助金额:$28.4万
-
财政年份:2019
-
负责人:Patrick Fragile
-
依托单位:
RUI: Numerical Simulations of Optically Thick Accretion onto Black Holes
-
批准号:1211230
-
项目类别:Standard Grant
-
资助金额:$18.97万
-
财政年份:2012
-
负责人:Patrick Fragile
-
依托单位:
RUI: Tilted Accretion Disks Around Rapidly Rotating Black Holes
-
批准号:0807385
-
项目类别:Standard Grant
-
资助金额:$15.52万
-
财政年份:2008
-
负责人:Patrick Fragile
-
依托单位:
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