gptkbp:instanceOf
|
dark matter
|
gptkbp:activeMass
|
62 kg
|
gptkbp:armament
|
gptkb:plastic
gptkb:water
gptkb:lead
copper
|
gptkbp:collaboratesWith
|
~100 scientists
|
gptkbp:country
|
gptkb:Italy
|
gptkbp:endDate
|
2016
|
gptkbp:foundIn
|
gptkb:WIMPs
gptkb:solar_neutrinos
dark photons
axions
magnetic monopoles
axion-like particles
neutrinoless double beta decay
bosonic dark matter
coherent neutrino-nucleus scattering
inelastic dark matter
light dark matter
solar axions
super-WIMPs
|
gptkbp:fundedBy
|
gptkb:National_Science_Foundation
gptkb:Weizmann_Institute_of_Science
gptkb:Deutsche_Forschungsgemeinschaft
gptkb:European_Research_Council
gptkb:INFN
|
gptkbp:goal
|
direct detection of dark matter
|
https://www.w3.org/2000/01/rdf-schema#label
|
XENON100 experiment
|
gptkbp:locatedIn
|
gptkb:Gran_Sasso_National_Laboratory
|
gptkbp:mass
|
161 kg
|
gptkbp:material
|
liquid xenon
|
gptkbp:notableAchievement
|
set world-leading limits on WIMP-nucleon cross-section
|
gptkbp:numberOfTubes
|
178
|
gptkbp:operatedBy
|
gptkb:XENON_collaboration
|
gptkbp:predecessor
|
gptkb:XENON10_experiment
|
gptkbp:publishedIn
|
gptkb:Physical_Review_Letters
gptkb:science
gptkb:Astroparticle_Physics
|
gptkbp:range
|
few keV to tens of keV
|
gptkbp:releaseDate
|
2011
2012
2016
|
gptkbp:sensitivity
|
~2 x 10^-45 cm^2 for WIMP-nucleon cross-section
|
gptkbp:sensorType
|
liquid xenon time projection chamber
|
gptkbp:startDate
|
2008
|
gptkbp:successor
|
gptkb:XENON1T_experiment
|
gptkbp:website
|
https://xenonexperiment.org/xenon100/
|
gptkbp:bfsParent
|
gptkb:XENON1T_experiment
|
gptkbp:bfsLayer
|
6
|