002674350 001__ 2674350
002674350 003__ SzGeCERN
002674350 005__ 20190514221553.0
002674350 0248_ $$aoai:inspirehep.net:1701586$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT$$pcerncds:CERN$$qINSPIRE:HEP$$qForCDS
002674350 035__ $$9http://inspirehep.net/oai2d$$aoai:inspirehep.net:1701586$$d2019-05-13T11:07:32Z$$h2019-05-14T04:02:55Z$$mmarcxml
002674350 035__ $$9Inspire$$a1701586
002674350 041__ $$aeng
002674350 100__ $$aUrbano, Alfredo$$uCERN
002674350 245__ $$aStrongly interacting light dark matter
002674350 260__ $$c2017
002674350 300__ $$a7 p
002674350 520__ $$9Grobid$$aWe discuss a class of Dark Matter (DM) models that, although inherently strongly coupled, appear weakly coupled at small-energy and fulfill the WIMP miracle, generating a sizable relic abundance through the standard freeze-out mechanism. Such models are based on approximate global symmetries that forbid relevant interactions; fundamental principles, like unitarity, restrict these symmetries to a small class, in such a way that the leading interactions between DM and the Standard Model are captured by effective operators up to dimension-8. The underlying strong coupling implies that these interactions become much larger at high-energy and represent an interesting novel target for LHC missing-energy searches.
002674350 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002674350 690C_ $$aCERN
002674350 773__ $$01700643$$c150-156$$pFrascati Phys. Ser.$$v65$$wC17-09-11.6$$y2017$$z9788886409612
002674350 8564_ $$81480243$$s764299$$uhttps://cds.cern.ch/record/2674350/files/1700643_150-156.pdf$$yFulltext
002674350 960__ $$a13
002674350 962__ $$b2320161$$k150-156$$ntrento20170911
002674350 980__ $$aARTICLE
002674350 980__ $$aConferencePaper
002674350 999C6 $$a0-0-1-1-0-0-0$$t2018-11-02 14:56:18$$vInvenio/1.1.2.1260-aa76f refextract/1.5.44$$vcontent.pdf;1
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