Speaker
Nikolina Ilic
(University of Toronto)
Description
The presence of a non-baryonic dark matter component in the Universe is inferred from the observation of its gravitational interaction. If dark matter interacts weakly with the Standard Model it would be produced at the LHC, escaping the detector and leaving a large missing transverse momentum as their signature. The ATLAS detector has developed a broad programme to directly search for DM. The results of recent searches on 13 TeV pp data, giving the details of analysis techniques and improvements used and their interpretation, will be presented
Primary authors
ATLAS Collaboration
Nikolina Ilic
(University of Toronto)
