| Project/Area Number |
20340039
|
|---|
| Research Category |
Grant-in-Aid for Scientific Research (B)
|
| Allocation Type | Single-year Grants |
|---|
| Section | 一般 |
|---|
| Research Field |
Astronomy
|
|---|
| Research Institution | Tohoku University |
|---|
Principal Investigator |
CHIBA Masashi 東北大学, 大学院・理学研究科, 教授 (50217246)
|
|---|
| Co-Investigator(Kenkyū-buntansha) |
INOUE Kaiki 近畿大学, 理工学部, 准教授 (70388495)
MINEZAKI Takeo 東京大学, 大学院・理学系研究科, 助教 (60292835)
|
|---|
| Co-Investigator(Renkei-kenkyūsha) |
SAITO Masao 国立天文台, ALMA推進室, 助教 (90353424)
KAMENO Seiji 鹿児島大学, 理学部, 准教授 (20270449)
SUGAI Hajime 京都大学, 大学院・理学研究科, 助教 (50291422)
SUMI Takahiro 名古屋大学, 太陽地球環境研究所, 助教 (30432214)
|
|---|
| Project Period (FY) |
2008 – 2010
|
| Project Status |
Completed (Fiscal Year 2010)
|
| Budget Amount *help |
¥16,250,000 (Direct Cost: ¥12,500,000、Indirect Cost: ¥3,750,000)
Fiscal Year 2010: ¥4,940,000 (Direct Cost: ¥3,800,000、Indirect Cost: ¥1,140,000)
Fiscal Year 2009: ¥4,940,000 (Direct Cost: ¥3,800,000、Indirect Cost: ¥1,140,000)
Fiscal Year 2008: ¥6,370,000 (Direct Cost: ¥4,900,000、Indirect Cost: ¥1,470,000)
|
|---|
| Keywords | 暗黒物質 / 電波観測 / 重力レンズ |
|---|
| Research Abstract |
Hierarchical clustering models of cold dark matter (CDM)predict that a galaxy-sized dark halo with total mass being comparable to the Milky Way contains thousands of substructures (so-called CDM subhalos)having each mass of million to billion solar masses. To directly identify such substructures and set limits on standard model of dark matter, we have developed the new method based on radio observation of gravitationally lensed objects using ALMA, TMT and other large-aperture telescopes with extremely high angular resolution.
|
