|
gptkbp:instanceOf
|
gptkb:scientific_research
|
|
gptkbp:alsoKnownAs
|
gptkb:Davis_Experiment
|
|
gptkbp:awardedBy
|
gptkb:Raymond_Davis_Jr.
|
|
gptkbp:country
|
gptkb:United_States
|
|
gptkbp:detectorMaterial
|
perchloroethylene
|
|
gptkbp:detectorVolume
|
615 tons
|
|
gptkbp:endDate
|
1994
|
|
gptkbp:field
|
astroparticle physics
neutrino physics
|
|
gptkbp:influenced
|
gptkb:Kamiokande_experiment
gptkb:Sudbury_Neutrino_Observatory
|
|
gptkbp:locatedIn
|
gptkb:Homestake_Gold_Mine
gptkb:Lead,_South_Dakota
|
|
gptkbp:maximumDepth
|
1,478 meters
|
|
gptkbp:method
|
chlorine detector
|
|
gptkbp:NobelPrizeYear
|
gptkb:2002_Nobel_Prize_in_Physics_(Raymond_Davis_Jr.)
|
|
gptkbp:notableFor
|
gptkb:solar_neutrino_problem
solar neutrino detection
|
|
gptkbp:principalInvestigator
|
gptkb:Raymond_Davis_Jr.
|
|
gptkbp:publishedIn
|
gptkb:Physical_Review_Letters
|
|
gptkbp:relatedTo
|
gptkb:solar_neutrino_problem
gptkb:Standard_Solar_Model
neutrino oscillation
|
|
gptkbp:result
|
first detection of solar neutrinos
observed neutrino deficit
|
|
gptkbp:startDate
|
1967
|
|
gptkbp:bfsParent
|
gptkb:solar_neutrino_problem
|
|
gptkbp:bfsLayer
|
5
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Homestake Experiment
|