Abstract
We present a complete particle physics model that explains three majorproblems of modern cosmology: inflation, dark matter and dark energy, andalso gives a mechanism for leptogenesis. The model has a new gauge groupSU(2)Z that growsstrong at a scale Λ ∼ 10−3 eV. We focus on the inflationary aspects of the model. Inflationoccurs with a Coleman–Weinberg potential at a low scale, down to∼ 6 × 105 GeV, being compatible with observational data.
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