Statements (56)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:scientific_experiments
|
| gptkbp:aims_to |
study neutrino properties
|
| gptkbp:can_provide |
data for theoretical models
|
| gptkbp:challenges |
current scientific paradigms
|
| gptkbp:collaborated_with |
other neutrino experiments
|
| gptkbp:collaborates_with |
international research institutions
|
| gptkbp:contribution |
neutrino physics
|
| gptkbp:depth |
700 meters
|
| gptkbp:designed_by |
gptkb:JUNO_collaboration
|
| gptkbp:enhances |
collaborative research efforts
|
| gptkbp:expansion_plans |
the frontiers of knowledge.
|
| gptkbp:facilitates |
future generations of physicists
young scientists in the field |
| gptkbp:fosters |
international scientific cooperation
|
| gptkbp:has_goal |
improve understanding of neutrino oscillation
|
| https://www.w3.org/2000/01/rdf-schema#label |
JUNO experiment
|
| gptkbp:include |
insights into the early universe
|
| gptkbp:investigates |
neutrino interactions
neutrino oscillation patterns neutrino production mechanisms |
| gptkbp:is_anticipated_by |
enhance knowledge of dark matter
|
| gptkbp:is_connected_to |
solar neutrinos
|
| gptkbp:is_examined_in |
neutrino flavor transitions
|
| gptkbp:is_expected_to |
new discoveries in particle physics
detect reactor antineutrinos measure neutrino mass hierarchy |
| gptkbp:is_expected_to_assess |
neutrino detection efficiency
|
| gptkbp:is_expected_to_characterize |
neutrino signal properties
|
| gptkbp:is_expected_to_detect |
antineutrinos from nuclear reactors
|
| gptkbp:is_expected_to_develop |
new detection technologies
|
| gptkbp:is_expected_to_evaluate |
neutrino background noise
|
| gptkbp:is_expected_to_measure |
neutrino mixing angles
neutrino energy spectra |
| gptkbp:is_expected_to_study |
neutrino decay processes
|
| gptkbp:is_expected_to_test |
theories of neutrino mass
|
| gptkbp:is_expected_to_validate |
existing neutrino models
|
| gptkbp:is_explored_in |
neutrino anomalies
|
| gptkbp:is_funded_by |
gptkb:Chinese_government
|
| gptkbp:is_involved_in |
neutrino astrophysics
|
| gptkbp:is_part_of |
China's neutrino program
global neutrino network |
| gptkbp:is_related_to |
supernova neutrinos
|
| gptkbp:is_significant_for |
fundamental physics research
|
| gptkbp:is_supported_by |
gptkb:scientific_community
|
| gptkbp:located_in |
gptkb:Jiangmen,_China
|
| gptkbp:mass |
20 kilotons
|
| gptkbp:notable_contributor |
astrophysics research
the search for new physics |
| gptkbp:promotes |
public understanding of science
|
| gptkbp:started_in |
gptkb:2021
|
| gptkbp:support |
theoretical predictions
|
| gptkbp:uses |
liquid scintillator
|
| gptkbp:uses_technology |
photomultiplier tubes
|
| gptkbp:utilizes |
advanced detection techniques
|
| gptkbp:bfsParent |
gptkb:Juno_Particle_Detector
|
| gptkbp:bfsLayer |
5
|