Statements (58)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:scientific_experiments
|
| gptkbp:analysis |
multi-channel analysis
|
| gptkbp:clinical_trial |
multi-year
|
| gptkbp:collaboration |
gptkb:2012
multinational team over 100 scientists Panda X Collaboration |
| gptkbp:collaborator |
gptkb:Chinese_Academy_of_Sciences
international scientists |
| gptkbp:collection |
scintillation light detection
|
| gptkbp:community_engagement |
outreach programs
|
| gptkbp:conference |
present findings
|
| gptkbp:data_type |
raw data
processed data |
| gptkbp:depth |
about 500 meters underground
|
| gptkbp:detector_design |
modular design
|
| gptkbp:detector_material |
xenon gas
|
| gptkbp:detector_volume |
1 ton
|
| gptkbp:environmental_impact |
minimal
|
| gptkbp:event_frequency |
low background events
|
| gptkbp:event_participation |
regular meetings
|
| gptkbp:experiment_challenges |
data interpretation
funding acquisition background noise reduction |
| gptkbp:experiment_phase |
Phase II
Phase III Phase I |
| gptkbp:field_of_study |
gptkb:Physics
astrophysics |
| gptkbp:first_run_year |
gptkb:2013
|
| gptkbp:focuses_on |
dark matter detection
|
| gptkbp:funding |
gptkb:National_Natural_Science_Foundation_of_China
approximately $10 million |
| gptkbp:future_plans |
expand research scope
collaborate with other experiments upgrade detector |
| gptkbp:goal |
search for weakly interacting massive particles (WIMPs)
|
| https://www.w3.org/2000/01/rdf-schema#label |
Panda X experiment
|
| gptkbp:impact |
high in dark matter research
|
| gptkbp:is_considered |
peer-reviewed process
|
| gptkbp:location |
gptkb:China
|
| gptkbp:neutrino_background |
reduced by depth
|
| gptkbp:operational_status |
ongoing
|
| gptkbp:provides_information_on |
open access
|
| gptkbp:publications |
Panda X collaboration papers
|
| gptkbp:release_frequency |
annual
|
| gptkbp:research |
LUX experiment
direct detection XENON experiment |
| gptkbp:safety_measures |
extensive safety protocols
|
| gptkbp:scientific_goals |
develop new technologies
improve sensitivity validate dark matter models |
| gptkbp:sensitivity |
sub-Ge V mass range
|
| gptkbp:sensor |
liquid xenon detector
|
| gptkbp:successor |
Panda X-4 T
|
| gptkbp:bfsParent |
gptkb:WIMPs
|
| gptkbp:bfsLayer |
5
|