| Co-Investigator(Kenkyū-buntansha) |
佐藤 修一 法政大学, 理工学部, 教授 (30425409)
田中 貴浩 京都大学, 理学研究科, 教授 (40281117)
武者 満 電気通信大学, レーザー新世代研究センター, 准教授 (40303028)
阿久津 智忠 国立天文台, 光赤外研究部, 助教 (40564274)
安東 正樹 東京大学, 大学院理学系研究科(理学部), 准教授 (90313197)
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| Budget Amount *help |
¥41,210,000 (Direct Cost: ¥31,700,000、Indirect Cost: ¥9,510,000)
Fiscal Year 2019: ¥7,800,000 (Direct Cost: ¥6,000,000、Indirect Cost: ¥1,800,000)
Fiscal Year 2018: ¥8,580,000 (Direct Cost: ¥6,600,000、Indirect Cost: ¥1,980,000)
Fiscal Year 2017: ¥7,670,000 (Direct Cost: ¥5,900,000、Indirect Cost: ¥1,770,000)
Fiscal Year 2016: ¥8,060,000 (Direct Cost: ¥6,200,000、Indirect Cost: ¥1,860,000)
Fiscal Year 2015: ¥9,100,000 (Direct Cost: ¥7,000,000、Indirect Cost: ¥2,100,000)
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| Outline of Final Research Achievements |
In the first year of this research, the first detection of the gravitational waves from coalescing binary black hole was presented by LIGO team. This research group A found that B-DECIGO which has a tenth of DECIGO in scale with the orbit around the earth can detect the gravitational waves from coalescing binary black holes up to almost the horizon of the universe. Following this fact, DECIGO group decided to adopt the road map of the project as B-DECIGO-->DECIGO which has 1000km in scale with the orbit around the sun. Key technology such as 1)test model of laser interferometer system on the earth 2) frequency stabilization of high power laser 3) drag free and control techniques of formation flight 4)designs of orbits have been developed so much.
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