| Budget Amount *help |
¥4,160,000 (Direct Cost: ¥3,200,000、Indirect Cost: ¥960,000)
Fiscal Year 2020: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2019: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2018: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2017: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
|
|---|
| Outline of Final Research Achievements |
The goal of this project is to propose concrete methods to detect dark matter of the Universe by focusing on the scalar sector including Higgs boson of the Standard Model. It was found that the pseudo-Nambu-Goldstone boson dark matter that interact with Higgs is hard detect in the future direct detection experiments, which indicates a new method required. For ultra-heavy dark matter, we simulated all kinds of cosmic-ray particles from dark matter in and outside the Galaxy. Consequently we found the gamma-ray and (anti)neutrino observations are most effective for the search of ultra-heavy dark matter.
|
