| Project/Area Number |
15K05088
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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 | Aoyama Gakuin University |
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Principal Investigator |
Yamazaki Ryo 青山学院大学, 理工学部, 准教授 (40420509)
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| Co-Investigator(Renkei-kenkyūsha) |
INOUE Tsuyoshi 名古屋大学, 大学院理学研究科, 准教授 (90531294)
OHIRA Yutaka 東京大学, 大学院理学系研究科, 助教 (40589347)
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| Project Period (FY) |
2015-04-01 – 2018-03-31
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| Project Status |
Completed (Fiscal Year 2017)
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| Budget Amount *help |
¥4,810,000 (Direct Cost: ¥3,700,000、Indirect Cost: ¥1,110,000)
Fiscal Year 2017: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2016: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2015: ¥2,470,000 (Direct Cost: ¥1,900,000、Indirect Cost: ¥570,000)
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| Keywords | 宇宙線 / 宇宙物理学 / 粒子加速 / 超新星残骸 / 無衝突衝撃波 / 宇宙物理 |
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| Outline of Final Research Achievements |
We studied theoretically and observationally shock waves propagating into realistic upstream medium, which are seen in, for example, supernova remnants. We performed X-ray and gamma-ray observations, and gave theoretical interpretations for them. Galaxy clusters and gravitational wave events are also studied in the context of the cosmic-ray acceleration.
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