Abstract
A cosmological first order electroweak phase transition could explain the origin of the matter-antimatter asymmetry in the Universe. Such a phase transition does not occur in the Standard Model, while it becomes possible with the existence of a second Higgs doublet in Nature. We obtain the properties of the new scalars , and that lead to such a phase transition, showing that its characteristic signature at LHC would be the observation of the decay . We analyze the LHC search prospects for this decay in the and final states, showing that either one is promising at the early stages of the 14 TeV run.
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