Statements (60)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:scientific_experiments
|
| gptkbp:aims_to_improve |
sensitivity to dark matter detection
|
| gptkbp:analysis |
multi-channel analysis
detector events |
| gptkbp:background_noise |
radioactive decay
|
| gptkbp:challenges |
background radiation interference
|
| gptkbp:collaboration |
with institutions worldwide
more than 100 scientists between physicists and engineers institutions from multiple countries |
| gptkbp:collaborator |
XENON collaboration
|
| gptkbp:collection |
2016 to 2020
|
| gptkbp:community_engagement |
to raise awareness about dark matter research
|
| gptkbp:community_outreach |
to educate the public
|
| gptkbp:contributes_to |
understanding of dark matter
|
| gptkbp:depth |
1,400 meters underground
|
| gptkbp:detector_mass |
3.2 tons
|
| gptkbp:first_results_released |
gptkb:2018
|
| gptkbp:funding |
from international grants
|
| gptkbp:future_plans |
for further experiments
|
| gptkbp:goal |
search for weakly interacting massive particles (WIMPs)
|
| gptkbp:has_data_sets |
available for analysis
|
| gptkbp:has_impact_on |
particle physics research
|
| gptkbp:has_meetings |
to discuss progress
|
| gptkbp:has_part |
liquid xenon target
|
| gptkbp:has_publications |
in scientific journals
|
| gptkbp:has_technical_reports |
documenting findings
|
| https://www.w3.org/2000/01/rdf-schema#label |
XENON1 T experiment
|
| gptkbp:influenced_by |
previous experiments like XENON100
|
| gptkbp:is_collaborative_research |
involving multiple disciplines
|
| gptkbp:is_considered |
a leading dark matter search experiment
|
| gptkbp:is_designed_to |
detect dark matter
|
| gptkbp:is_documented_in |
gptkb:literature
|
| gptkbp:is_evaluated_by |
peer review process
|
| gptkbp:is_funded_by |
gptkb:European_Research_Council
|
| gptkbp:is_monitored_by |
scientific committees
|
| gptkbp:is_part_of |
larger dark matter research efforts
the XENON project series |
| gptkbp:is_recognized_for |
its contributions to astrophysics
|
| gptkbp:is_supported_by |
various scientific organizations
|
| gptkbp:is_utilized_in |
educational programs.
|
| gptkbp:located_in |
Gran Sasso National Laboratory
|
| gptkbp:measures |
scintillation light
|
| gptkbp:notable_work |
exclusion limits on dark matter interactions
|
| gptkbp:operational_status |
completed data taking
|
| gptkbp:primary_use |
detecting rare events
|
| gptkbp:result |
gptkb:2020
|
| gptkbp:sensitivity |
sub-Ge V dark matter
|
| gptkbp:specification |
detailed in research papers
|
| gptkbp:started_in |
gptkb:2016
|
| gptkbp:successor |
XENONn T
|
| gptkbp:type_of_detection |
noble liquid detection
|
| gptkbp:uses |
liquid xenon
|
| gptkbp:uses_calibration_methods |
to ensure accuracy
|
| gptkbp:uses_cryogenics |
to maintain low temperatures
|
| gptkbp:uses_photomultiplier_tubes |
for light detection
|
| gptkbp:uses_technology |
time projection chamber
|
| gptkbp:utilizes |
advanced data acquisition systems
|
| gptkbp:bfsParent |
gptkb:WIMPs
|
| gptkbp:bfsLayer |
5
|