Gravitational waves from the remnants of primordial stars
| Project/Area Number |
16H06715
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| Research Category |
Grant-in-Aid for Research Activity Start-up
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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 |
Kinugawa Tomoya 東京大学, 宇宙線研究所, 特任研究員 (90779159)
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| Project Period (FY) |
2016-08-26 – 2018-03-31
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| Project Status |
Completed (Fiscal Year 2017)
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| Budget Amount *help |
¥2,600,000 (Direct Cost: ¥2,000,000、Indirect Cost: ¥600,000)
Fiscal Year 2017: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2016: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
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| Keywords | 連星進化 / 初代星 / 重力波 / 金属量進化 / ブラックホール / 宇宙物理 / 理論天文学 |
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| Outline of Final Research Achievements |
I researched binary evolutions and expected what kind of binaries will be observed. I wrote papers such as the neutron star - black hole binary of first star for gravitational wave observation, whether the binary black hole of first star ca distinguish from the binary black hole formed at the present day, and the gamma ray burst rate of the binary merger model.
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Report
(3 results)
Research Products
(15 results)
