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 language||English (US)|
|Journal||EPJ Web of Conferences|
|State||Published - Mar 23 2017|
|Event||6th Roma International Conference on Astroparticle Physics, RICAP 2016 - Frascati, Roma, Italy|
Duration: Jun 21 2016 → Jun 24 2016