Study of the accretion flow onto super-spinars
| Project/Area Number |
22740147
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | The University of Tokyo |
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Principal Investigator |
BAMBI Cosimo 東京大学, 数物連携宇宙研究機構, 特任研究員 (30534995)
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| Project Period (FY) |
2010 – 2011
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| Project Status |
Completed (Fiscal Year 2011)
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| Budget Amount *help |
¥3,510,000 (Direct Cost: ¥2,700,000、Indirect Cost: ¥810,000)
Fiscal Year 2011: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2010: ¥1,950,000 (Direct Cost: ¥1,500,000、Indirect Cost: ¥450,000)
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| Keywords | 相対論 / 重力(理論) |
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| Research Abstract |
The final product of the gravitational collapse is thought to be a black hole and astronomers have discovered several good astrophysical candidates. In order to confirm this conjecture, we need to probe the geometry of the space-time around these objects and check it is consistent with the predictions of General Relativity. My project has studied how present and near-future sub-millimeter and X-ray data can test the actual nature of the current astrophysical black hole candidates.
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Report
(3 results)
Research Products
(27 results)
