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Dark energy, the electroweak vacua and collider phenomenology

2008/10/31 by Eric Greenwood, Evan Halstead, Robert Poltis +1
Physics and Astronomy · #hep-ph #astro-ph #gr-qc

paper · pdf · doi:10.1103/physrevd.79.103003

published as Phys.Rev.D79:103003,2009 · Expanded version. Published in Phys. Rev. D

arxiv created 2009/05/12 · arxiv updated 2010/04/21

Abstract

Higher dimensional non-renormalizable 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 the 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 kink-like 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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