gptkbp:instanceOf
|
neutrino
|
gptkbp:awardedBy
|
gptkb:Takaaki_Kajita
|
gptkbp:collaboratesWith
|
international
|
gptkbp:country
|
gptkb:Japan
|
gptkbp:fundedBy
|
international partners
Japanese government
|
https://www.w3.org/2000/01/rdf-schema#label
|
Super-Kamiokande
|
gptkbp:location
|
gptkb:Hida,_Gifu_Prefecture,_Japan
|
gptkbp:maximumDepth
|
1000 meters underground
|
gptkbp:notableFinds
|
gptkb:atmospheric_neutrino_anomaly
evidence for neutrino oscillations
|
gptkbp:notableRelease
|
gptkb:Super-Kamiokande-Gd
|
gptkbp:opened
|
1996
|
gptkbp:operatedBy
|
gptkb:Institute_for_Cosmic_Ray_Research,_University_of_Tokyo
|
gptkbp:photomultiplierTubes
|
over 11,000
|
gptkbp:predecessor
|
gptkb:Kamiokande
|
gptkbp:purpose
|
study of neutrino oscillations
detection of supernova neutrinos
search for proton decay
|
gptkbp:relatedTo
|
gptkb:Hyper-Kamiokande
gptkb:Kamioka_Observatory
gptkb:Nobel_Prize_in_Physics_2015
|
gptkbp:sensorType
|
water Cherenkov detector
|
gptkbp:status
|
operational
|
gptkbp:tankVolume
|
50,000 tons
|
gptkbp:website
|
http://www-sk.icrr.u-tokyo.ac.jp/sk/index-e.html
|
gptkbp:bfsParent
|
gptkb:neutrinos
gptkb:solar_neutrino_problem
gptkb:T2K_experiment
gptkb:neutrino
|
gptkbp:bfsLayer
|
5
|