gptkbp:instance_of
|
gptkb:Nexon
|
gptkbp:capacity
|
50,000 tons
|
gptkbp:collaborated_with
|
SNO experiment
|
gptkbp:collaboration
|
gptkb:Super-Kamiokande_Collaboration
|
gptkbp:collection
|
ongoing
|
gptkbp:depth
|
1,000 meters
|
gptkbp:designed_to_detect
|
gptkb:Nexon
|
gptkbp:discovery
|
atmospheric neutrino oscillation
|
gptkbp:field_of_study
|
gptkb:Physics
|
gptkbp:has_method
|
Cherenkov radiation
|
gptkbp:has_publications
|
over 1,000
|
gptkbp:has_research_focus
|
gptkb:Quantum_Mechanics
gptkb:Physics
gptkb:cosmology
astrophysics
nuclear physics
cosmic rays
high-energy physics
relativity
experimental physics
neutrino interactions
neutrino mass
neutrino astrophysics
neutrino detectors
neutrino experiments
neutrino flavor
neutrino properties
neutrino mixing
particle astrophysics
neutrino oscillation experiments
neutrino sources
dark matter candidates
neutrino detection technology
fundamental symmetries
cosmic neutrinos
CP violation in neutrinos
proton decay
|
gptkbp:has_subdetector
|
gptkb:Super-Kamiokande_IV
gptkb:Super-Kamiokande_II
gptkb:Super-Kamiokande_III
|
https://www.w3.org/2000/01/rdf-schema#label
|
Super-Kamiokande detector
|
gptkbp:impact
|
neutrino physics
|
gptkbp:is_funded_by
|
gptkb:Japanese_government
|
gptkbp:location
|
gptkb:Kamioka,_Japan
|
gptkbp:measures
|
atmospheric neutrinos
solar neutrinos
supernova neutrinos
|
gptkbp:number_of_photomultiplier_tubes
|
11,146
|
gptkbp:operated_by
|
gptkb:Institute_for_Cosmic_Ray_Research
|
gptkbp:operational_since
|
gptkb:1996
|
gptkbp:type
|
large water Cherenkov detector
|
gptkbp:uses
|
water Cherenkov detection
|
gptkbp:bfsParent
|
gptkb:T2_K_Collaboration
|
gptkbp:bfsLayer
|
5
|