002750413 001__ 2750413
002750413 003__ SzGeCERN
002750413 005__ 20210209110745.0
002750413 0247_ $$2DOI$$9IOP$$a10.1088/1742-6596/1690/1/012153
002750413 0248_ $$aoai:inspirehep.net:1838727$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002750413 035__ $$9http://old.inspirehep.net/oai2d$$aoai:inspirehep.net:1838727$$d2021-01-26T14:26:28Z$$h2021-01-27T05:00:04Z$$mmarcxml
002750413 035__ $$9Inspire$$a1838727
002750413 041__ $$aeng
002750413 100__ $$aIlic, N$$uCERN
002750413 245__ $$9IOP$$aSearching for Dark Matter with the ATLAS detector
002750413 260__ $$c2020
002750413 300__ $$a6 p
002750413 520__ $$9IOP$$aThe presence of a non-baryonic dark matter component in the Universe is inferred from the observation of its gravitational interaction. If dark matter interacts weakly with the Standard Model it would be produced at the LHC, escaping the detector and leaving a large missing transverse momentum as their signature. The ATLAS detector has developed a broad program to directly search for Dark Matter. The results of recent searches on 13 TeV pp data, giving the details of analysis techniques and improvements used and their interpretation, are presented.
002750413 540__ $$aCC-BY-3.0$$bIOP$$uhttp://creativecommons.org/licenses/by/3.0
002750413 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002750413 690C_ $$aCERN
002750413 693__ $$aCERN LHC$$eATLAS
002750413 710__ $$gATLAS Collaboration
002750413 773__ $$01838300$$c012153$$n1$$pJ. Phys.: Conf. Ser.$$v1690$$wC20-10-05$$y2020
002750413 8564_ $$82275110$$s1402803$$uhttps://cds.cern.ch/record/2750413/files/Ilic_2020_J._Phys.__Conf._Ser._1690_012153.pdf$$yFulltext
002750413 960__ $$a13
002750413 962__ $$b2718781$$k012153$$nmoscow20201005
002750413 980__ $$aARTICLE
002750413 980__ $$aConferencePaper