| Budget Amount *help |
¥119,990,000 (Direct Cost: ¥92,300,000、Indirect Cost: ¥27,690,000)
Fiscal Year 2016: ¥23,400,000 (Direct Cost: ¥18,000,000、Indirect Cost: ¥5,400,000)
Fiscal Year 2015: ¥23,400,000 (Direct Cost: ¥18,000,000、Indirect Cost: ¥5,400,000)
Fiscal Year 2014: ¥26,390,000 (Direct Cost: ¥20,300,000、Indirect Cost: ¥6,090,000)
Fiscal Year 2013: ¥20,540,000 (Direct Cost: ¥15,800,000、Indirect Cost: ¥4,740,000)
Fiscal Year 2012: ¥26,260,000 (Direct Cost: ¥20,200,000、Indirect Cost: ¥6,060,000)
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| Outline of Final Research Achievements |
Core collapse supernova explosions are among the most dramatic and important events to take place in the universe. This research is a study of the correlation between neutrino and gravitational wave by supernova explosion, and aimed at developing the world's most advanced-technology supernova neutrino detector. In April 2015, the EGADS detector has been full of water enriched with 0.2% gadolinium sulfate, equipped with new electronic circuits and computers, and began operation as a water Cherenkov detector capable of neutron capture with high efficiency. In addition, we studied the prediction of signal correlation of neutrino and gravitational wave when neighboring supernovae occurred.
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