Physics of dark matter and 130GeV gamma-ray signal
Project/Area Number |
25400262
|
Research Category |
Grant-in-Aid for Scientific Research (C)
|
Allocation Type | Multi-year Fund |
Section | 一般 |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
Research Institution | University of the Ryukyus |
Principal Investigator |
Oda Ichiro 琉球大学, 理学部, 教授 (40265517)
|
Co-Investigator(Kenkyū-buntansha) |
URYU Koji 琉球大学, 理学部, 教授 (40457693)
|
Project Period (FY) |
2013-04-01 – 2016-03-31
|
Project Status |
Completed (Fiscal Year 2015)
|
Budget Amount *help |
¥3,900,000 (Direct Cost: ¥3,000,000、Indirect Cost: ¥900,000)
Fiscal Year 2015: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2014: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2013: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
|
Keywords | 暗黒物質 / 標準理論を超える理論 / ブラックホール / ホーキング輻射 / コンフォーマルな重力 / 標準模型 / ヒッグス粒子 / Bモード |
Outline of Final Research Achievements |
One of the biggest mysteries in both modern elementary particle physics and cosmology is on physics of dark matter. Owing to the recent progress of observation, it turned out that the total energy of our university is consisted of about 75% dark energy, about 25% dark matter and the remaining about 5% ordinary matters. One of purposes of our study is to clarify the physics of the dark matter on the basis of 130 GeV gamma-rays which were observed by the fermi satellite.
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Report
(4 results)
Research Products
(9 results)