Speaker
Dr
Yusuke Koshio
(Kamioka observatory, ICRR, Univ. of Tokyo)
Description
The sensitivity of solar neutrinos is discussed in this presentation. The modification from the previous meeting will be updated back ground rate from spallation, therefore, the results will be more realistic. Another topics is supernova burst neutrinos. This will be more precise than the discussion in the previous meeting, especially, a correlation with another observation such as gravitational wave.
Primary author
Dr
Yusuke Koshio
(Kamioka observatory, ICRR, Univ. of Tokyo)
