Speaker
Mario Gomez
(Universidad de Huelva)
Description
We will review the expectations for LFV, LHC and dark matter searches, for different grand unification groups, paying particular attention to the comparison between their distinct signatures, and to ways to differentiate between the various schemes in present and future searches. Since SO(10) is by now already too constrained by the data, we will focus on SU(5), flipped SU(5) and SU(4)c × SU(2)L ×SU(2)R (4-2-2). Similarly to previous works for various GUTs, we assume that at the unification scale the SUSY soft terms still preserve the group symmetry, and focus on the effects derived from the gauge structure of the groups.
