Study for the cosmic-ray interaction with Earth's atmosphere using LHC nuclear collisions
| Project/Area Number |
20740130
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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 | Nagoya University |
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Principal Investigator |
SAKO Takashi Nagoya University, 太陽地球環境研究所, 助教 (90324368)
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| Research Collaborator |
KAWADE Kentaro 名古屋大学, 大学院・理学研究科, 大学院生
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| Project Period (FY) |
2008 – 2009
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| Project Status |
Completed (Fiscal Year 2009)
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| Budget Amount *help |
¥4,290,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥990,000)
Fiscal Year 2009: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
Fiscal Year 2008: ¥2,470,000 (Direct Cost: ¥1,900,000、Indirect Cost: ¥570,000)
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| Keywords | 超高エネルギー宇宙線 / 相互作用モデル / シンチレータ / LHC原子核衝突 / 宇宙線 / 宇宙物理 / 加速器 / 放射線、X線、粒子線 / 最高エネルギー宇宙線 / LHC加速器 / ハドロン相互作用 |
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| Research Abstract |
We investigated future experiments to test interaction models using nuclear collisions at the CERN LHC accelerator. In point of view of the model discrimination, particle multiplicity and radiation dose, we concluded that we can perform a crucial experiment at Nitrogen collisions, but not at the Lead collisions assuming to use the current LHCf detector. We also studied the basic properties of GSO crystal scintillator to reduce the radiation damage. We concluded that the GSO scintillators are radiation hard enough and have satisfactory properties compared with the plastic scintillators used in the current detector.
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Report
(3 results)
Research Products
(9 results)
