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arxiv: 1009.5099 · v1 · pith:5VMFBYNOnew · submitted 2010-09-26 · ✦ hep-ph

Inert Model and evolution of the Universe

classification ✦ hep-ph
keywords inertphasedarkevolutionleadinguniverseaddressboson
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We consider evolution of the Universe after EWSB leading to the present inert phase, containing a SM-like Higgs boson and scalar dark particles, among them a Dark Matter candidate. We address the question, if there is a possibility to have a sequence of the phase transitions instead of a single one leading directly from EW symmetric phase to the inert one.

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