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SUMMARY:Solar neutrino results from Super-Kamiokande
DTSTART;VALUE=DATE-TIME:20120705T234500Z
DTEND;VALUE=DATE-TIME:20120706T000000Z
DTSTAMP;VALUE=DATE-TIME:20130525T035727Z
UID:indico-contribution-121@cern.ch
DESCRIPTION:Speakers: Dr. KOSHIO\, Yusuke (Kamioka observatory  ICRR Unive
 rsity of Tokyo (JP))\nRecent results of the Super-Kamiokande (SK) solar ne
 utrino measurements are presented. The main goal of SK's solar analysis is
  to observe the MSW effect\, i.e. a solar neutrino energy spectrum distort
 ion induced by matter in the Sun\, and a day/night solar neutrino flux asy
 mmetry induced by matter in the Earth.\n Thanks to the improvement of the 
 detector's water circulation system\, low energy background levels have be
 en reduced and clear solar neutrino signals are seen even for 4.0-4.5MeV e
 lectron kinetic energy range\, along with some indications of a signal eve
 n down to 3.5-4.0MeV.\n The combined energy spectrum and day/night solar n
 eutrino flux from phase I to phase IV in SK will be presented. A global os
 cillation analysis has been carried out using SK-I\, II\, III\, and IV dat
 a and combining these results with the results of other solar neutrino exp
 eriments as well as the KamLAND reactor experiment.  The results of this g
 lobal analysis will also be presented.\n\nhttp://indico.cern.ch/contributi
 onDisplay.py?contribId=121&sessionId=71&confId=181298
LOCATION:Melbourne Convention and Exhibition Centre Room 220
URL:http://indico.cern.ch/contributionDisplay.py?contribId=121&sessionId=7
 1&confId=181298
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