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SUMMARY:Atmospheric neutrino oscillation in Super-Kamiokande
DTSTART;VALUE=DATE-TIME:20070707T174100Z
DTEND;VALUE=DATE-TIME:20070707T175300Z
DTSTAMP;VALUE=DATE-TIME:20261011T153901Z
UID:indico-contribution-1097@cern.ch
DESCRIPTION:Speakers: Ms. TAKENAGA\, Yumiko (ICRR\, University of Tokyo)\n
 The Super-Kamiokande started observation in April of 1996 and continued th
 e \ndata taking for five years of initial running period (SK-I) till the m
 aintenance in \nJuly of 2001. The Super-Kamiokande continued the data taki
 ng with the half \nPMT density in the second period (SK-II) from resuming 
 in December of 2002 to \nshutdown for the reconstruction to return the PMT
  density in October 2005. \nUsing the atmospheric neutrino data of SK-I an
 d SK-II\, various types of \noscillation analyses have been performed.\nTh
 e results from the nu_mu  nu_tau 2 flavor oscillation analysis and the 3 \
 nflavor oscillation analysis with the aim of searching for a non-zero 1-3 
 mixing \nwill be presented. The results from an oscillation analysis inclu
 ding the sub-\ndominant oscillation effects driven by the solar oscillatio
 n terms (theta_12 and \ndm^2_12) will also be reported.\n\nhttps://indico.
 nucleares.unam.mx/event/4/session/63/contribution/1097
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/63/contribution/1097
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