2015 Fiscal Year Final Research Report
Theoretical Study for the detection of Astrophysical Black Hole Spacetime
| Project/Area Number |
24540268
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Multi-year Fund |
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| Section | 一般 |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | Aichi University of Education |
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Principal Investigator |
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| Project Period (FY) |
2012-04-01 – 2016-03-31
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| Keywords | ブラックホール / 一般相対論 / 磁気流体力学 / 高エネルギー天体現象 / サブミリ波VLBI観測 / 衝撃波 / ガンマ線バースト / S２天体の近日点移動 |
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| Outline of Final Research Achievements |
The structure of magnetosphere of a black hole is studied to understand the high-energy astrophysical phenomena in active galactic nuclei and some compact X-ray sources. Such high-energy phenomena are due to a massive black hole with magnetized plasma accretion, where the effects of strong gravity (i.e., the general relativistic effects) have a crucial role in the system around the black hole. I and collaborators make a project to detect some information about the black hole's curved spacetime by radio VLBI observation and near-infrared observation.
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| Free Research Field |
宇宙物理学
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