Statements (58)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:physicist
|
| gptkbp:aims_to |
sensitivity to dark matter detection
|
| gptkbp:analysis |
multi-channel analysis
detector events |
| gptkbp:challenges |
background radiation interference
|
| gptkbp:collaborations |
with institutions worldwide
to discuss progress more than 100 scientists XENON collaboration between physicists and engineers institutions from multiple countries involving multiple disciplines |
| gptkbp:collection |
2016 to 2020
|
| gptkbp:community_engagement |
to raise awareness about dark matter research
|
| gptkbp:community_involvement |
to educate the public
|
| gptkbp:contributed_to |
understanding of dark matter
|
| gptkbp:depth |
1,400 meters underground
|
| gptkbp:first_released |
gptkb:2018
|
| gptkbp:future_plans |
for further experiments
|
| gptkbp:goal |
search for weakly interacting massive particles (WIM Ps)
|
| gptkbp:has_collection |
available for analysis
|
| gptkbp:has_documentation |
documenting findings
|
| gptkbp:has_impact_on |
particle physics research
|
| gptkbp:has_part |
liquid xenon target
|
| https://www.w3.org/2000/01/rdf-schema#label |
XENON1 T experiment
|
| gptkbp:influenced_by |
previous experiments like XENO N100
|
| gptkbp:instrumentation |
to ensure accuracy
|
| gptkbp:is_considered |
a leading dark matter search experiment
|
| gptkbp:is_designed_to |
detect dark matter
|
| gptkbp:is_documented_in |
gptkb:literary_work
|
| gptkbp:is_evaluated_by |
peer review process
|
| 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_used_by |
to maintain low temperatures
|
| gptkbp:is_utilized_in |
educational programs.
|
| gptkbp:launched |
gptkb:2016
|
| gptkbp:located_in |
Gran Sasso National Laboratory
|
| gptkbp:mass |
3.2 tons
|
| gptkbp:measures |
scintillation light
|
| gptkbp:noise_level |
radioactive decay
|
| gptkbp:notable_work |
exclusion limits on dark matter interactions
|
| gptkbp:operational_status |
completed data taking
|
| gptkbp:photography |
for light detection
|
| gptkbp:primary_source |
detecting rare events
|
| gptkbp:publishes |
in scientific journals
|
| gptkbp:receives_funding_from |
gptkb:European_Research_Council
from international grants |
| gptkbp:recognizes |
noble liquid detection
|
| gptkbp:result |
gptkb:2020
|
| gptkbp:sensor |
sub-Ge V dark matter
|
| gptkbp:specifies |
detailed in research papers
|
| gptkbp:successor |
XENO Nn T
|
| gptkbp:technology |
time projection chamber
|
| gptkbp:uses |
liquid xenon
|
| gptkbp:utilizes |
advanced data acquisition systems
|