Higher dimensional nonrenormalizable operators may modify the standard model Higgs potential in many interesting ways. Here, we consider the appearance of a second vacuum which may play an important role in cosmology. For a certain range of parameters, the usual second-order electroweak phase transition is followed by a first-order phase transition that may drive the late time accelerated expansion of the Universe. Such a potential contains kinklike solutions which in turn can play a crucial role in reconstructing the global shape of the potential in colliders, as we explicitly demonstrate.
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Greenwood et al. (2009) studied this question.
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