21-23 August 2012
Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), The University of Tokyo
Asia/Tokyo timezone

Solar neutrinos and supernova burst neutrinos at Hyper-Kamiokande

22 Aug 2012, 16:25
25m
Lecture Hall (Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), The University of Tokyo)

Lecture Hall

Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), The University of Tokyo

5-1-5 Kashiwanoha, Kashiwa city, Chiba, 277-8583 JAPAN

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)

Presentation Materials

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