Speaker
Dr
Yusuke Koshio
(Kamioka observatory, ICRR, Univ. of Tokyo)
Description
n this presentation, the sensitivity of solar neutrinos is discussed. In the case of shallow place, the most serious background will be spallation products induced from cosmic ray muons. How much reduce background by improving an analysis method will be estimated. Using this result, the requirement for the solar neutrino physics, such as the constraint to delta-m-square_21, is discussed. The expectation event rate from the SuperNova burst is also discussed.
Primary author
Dr
Yusuke Koshio
(Kamioka observatory, ICRR, Univ. of Tokyo)
