| Budget Amount *help |
¥57,850,000 (Direct Cost: ¥44,500,000、Indirect Cost: ¥13,350,000)
Fiscal Year 2018: ¥8,320,000 (Direct Cost: ¥6,400,000、Indirect Cost: ¥1,920,000)
Fiscal Year 2017: ¥12,480,000 (Direct Cost: ¥9,600,000、Indirect Cost: ¥2,880,000)
Fiscal Year 2016: ¥20,280,000 (Direct Cost: ¥15,600,000、Indirect Cost: ¥4,680,000)
Fiscal Year 2015: ¥11,960,000 (Direct Cost: ¥9,200,000、Indirect Cost: ¥2,760,000)
Fiscal Year 2014: ¥4,810,000 (Direct Cost: ¥3,700,000、Indirect Cost: ¥1,110,000)
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| Outline of Final Research Achievements |
We aim to study of the most energetic phenomena, supernova, from observations of nearby supernovae. KamLAND developed the unique supernova alarm system that used pre-supernova neutrinos emitted from nearby starts in core burning phase. Based on recent progresso of astronomical observations and theory of stellar evolution, we established modern pre-supernova neutrino model. SK, KamLAND and XMASS updated their DAQ system for nearby supernovae and made a success of stable observations for supernovae. We started the collaboration with not only the Kamioka group, but also world-wide neutrino and gravitational wave detectors.
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