Dark Matter after LHC Run I: Clues to Unification

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After the results of Run I, can we still 'guarantee' the discovery of supersymmetry at the LHC? It is shown that viable dark matter models in CMSSM-like models tend to lie in strips (co-annihilation, funnel, focus point). The role of grand unification in constructing supersymmetric models is discussed and it is argued that non-supersymmetric GUTs such as SO(10) may provide solutions to many of the standard problems addressed by supersymmetry.

Original languageEnglish (US)
Article number01001
JournalEPJ Web of Conferences
StatePublished - Mar 23 2017
Event6th Roma International Conference on Astroparticle Physics, RICAP 2016 - Frascati, Roma, Italy
Duration: Jun 21 2016Jun 24 2016

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