gptkbp:instanceOf
|
scientific research
|
gptkbp:aimsTo
|
search for dark matter
detect axions
|
gptkbp:collaboratesWith
|
gptkb:treaty
|
gptkbp:country
|
gptkb:United_States
|
gptkbp:field
|
physics
|
gptkbp:fullName
|
gptkb:Axion_Dark_Matter_Experiment
|
gptkbp:fundedBy
|
gptkb:National_Science_Foundation
gptkb:U.S._Department_of_Energy
|
https://www.w3.org/2000/01/rdf-schema#label
|
ADMX experiment
|
gptkbp:location
|
gptkb:University_of_Washington
|
gptkbp:notableAchievement
|
improved sensitivity for axion detection
set limits on axion mass
|
gptkbp:partner
|
gptkb:Fermi_National_Accelerator_Laboratory
gptkb:Lawrence_Livermore_National_Laboratory
gptkb:Los_Alamos_National_Laboratory
gptkb:Pacific_Northwest_National_Laboratory
gptkb:University_of_California,_Berkeley
gptkb:University_of_Florida
gptkb:University_of_Sheffield
gptkb:University_of_Washington
|
gptkbp:principalInvestigator
|
gptkb:Gray_Rybka
|
gptkbp:releaseDate
|
publications in Physical Review Letters
|
gptkbp:researchArea
|
dark matter
axion detection
|
gptkbp:sensorType
|
haloscope
|
gptkbp:startDate
|
1996
|
gptkbp:status
|
operational
|
gptkbp:technology
|
microwave cavity
superconducting magnet
|
gptkbp:website
|
https://admx.io/
|
gptkbp:bfsParent
|
gptkb:axion
|
gptkbp:bfsLayer
|
6
|