|
gptkbp:instanceOf
|
Particle
|
|
gptkbp:antiparticle
|
neutrino
|
|
gptkbp:charge
|
0
|
|
gptkbp:communicatesVia
|
gptkb:Weak_interaction
Gravity
|
|
gptkbp:compatibleWith
|
gptkb:Electromagnetic_interaction
gptkb:Strong_interaction
|
|
gptkbp:detects
|
gptkb:IceCube_Neutrino_Observatory
gptkb:Sudbury_Neutrino_Observatory
gptkb:Super-Kamiokande
Neutrino observatories
|
|
gptkbp:discoveredBy
|
gptkb:Frederick_Reines
gptkb:Clyde_Cowan
|
|
gptkbp:discoveredIn
|
1956
|
|
gptkbp:family
|
Fermion
|
|
gptkbp:hasType
|
gptkb:Electron_neutrino
gptkb:Muon_neutrino
gptkb:Tau_neutrino
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Neutrinos
|
|
gptkbp:isFermion
|
true
|
|
gptkbp:isLepton
|
true
|
|
gptkbp:isStandardModelParticle
|
true
|
|
gptkbp:lifespan
|
Stable
|
|
gptkbp:mass
|
Very small, nonzero
|
|
gptkbp:meanFreePath
|
Extremely long
|
|
gptkbp:nameOrigin
|
Italian for 'little neutral one'
|
|
gptkbp:numberOfFlavors
|
3
|
|
gptkbp:oscillatesBetweenFlavors
|
true
|
|
gptkbp:penetration
|
Very high
|
|
gptkbp:producedBy
|
gptkb:Cosmic_rays
Sun
Nuclear reactors
Nuclear reactions
Supernovae
|
|
gptkbp:proposedBy
|
gptkb:Wolfgang_Pauli
|
|
gptkbp:relatedTo
|
gptkb:Solar_neutrino_problem
gptkb:Neutrinoless_double_beta_decay
Beta decay
Neutrino oscillation
Dark matter (possible connection)
|
|
gptkbp:roleInCosmology
|
Affects structure formation
|
|
gptkbp:roleInPhysics
|
Evidence for physics beyond Standard Model
|
|
gptkbp:spin
|
1/2
|
|
gptkbp:statistic
|
gptkb:Fermi-Dirac
|
|
gptkbp:subjectOf
|
gptkb:Nobel_Prize_in_Physics_2015
gptkb:Nobel_Prize_in_Physics_1995
gptkb:Nobel_Prize_in_Physics_2002
|
|
gptkbp:symbol
|
ν
|
|
gptkbp:yearProposed
|
1930
|
|
gptkbp:bfsParent
|
gptkb:Electromagnetic_Calorimeter
|
|
gptkbp:bfsLayer
|
5
|