|
gptkbp:instanceOf
|
Particle
|
|
gptkbp:antiparticle
|
neutrino
|
|
gptkbp:canChangeFlavor
|
true
|
|
gptkbp:communicatesVia
|
gptkb:weak_nuclear_force
gravity
|
|
gptkbp:compatibleWith
|
gptkb:electromagnetic_force
gptkb:strong_nuclear_force
|
|
gptkbp:detects
|
neutrino observatories
|
|
gptkbp:discoveredBy
|
gptkb:Frederick_Reines
gptkb:Clyde_Cowan
|
|
gptkbp:discoveredIn
|
1956
|
|
gptkbp:flavor
|
gptkb:tau_neutrino
gptkb:electron_neutrino
muon neutrino
|
|
gptkbp:hasRestMass
|
very small, nonzero
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
neutrinos
|
|
gptkbp:isAbundantIn
|
universe
|
|
gptkbp:isFermion
|
true
|
|
gptkbp:isLepton
|
true
|
|
gptkbp:isNeutral
|
true
|
|
gptkbp:lifespan
|
gptkb:standard
|
|
gptkbp:massUpperLimit
|
less than 1 eV/c^2
|
|
gptkbp:partOf
|
gptkb:Standard_Model
|
|
gptkbp:penetration
|
very high
|
|
gptkbp:predictionYear
|
1930
|
|
gptkbp:predicts
|
gptkb:Wolfgang_Pauli
|
|
gptkbp:producedBy
|
cosmic rays
nuclear reactions
sun
supernovae
|
|
gptkbp:range
|
0
|
|
gptkbp:spin
|
1/2
|
|
gptkbp:subjectOf
|
gptkb:IceCube_Neutrino_Observatory
gptkb:solar_neutrino_problem
gptkb:Borexino_experiment
gptkb:Daya_Bay_Reactor_Neutrino_Experiment
gptkb:KATRIN_experiment
gptkb:KamLAND
gptkb:MINOS_experiment
gptkb:NOvA_experiment
gptkb:OPERA_experiment
gptkb:Sudbury_Neutrino_Observatory
gptkb:Super-Kamiokande
gptkb:T2K_experiment
neutrino astronomy
double beta decay
neutrino mass measurement
neutrino oscillation
neutrino oscillation experiments
|
|
gptkbp:symbol
|
ν
|
|
gptkbp:bfsParent
|
gptkb:CNO_cycle
gptkb:Fermi-Dirac_statistics
|
|
gptkbp:bfsLayer
|
4
|