Low-scale inflation in a model of dark energy and dark matter

Details Low-scale inflation in a model of dark energy and dark matter Low-scale inflation in a model of dark energy and dark matter

2006-09-28

arxiv.org/abs/astro-ph/0609777v2

JCAP0612:004,2006

Astronomy and Astrophysics

Astrophysics

5 two-column pages, RevTex4; two reference added and minor changes made in the text; published in JCAP

Scientific paper

10.1088/1475-7516/2006/12/004

We present a complete particle physics model that explains three major problems of modern cosmology: inflation, dark matter and dark energy, and also gives a mechanism for leptogenesis. The model has a new gauge group $SU(2)_Z$ that grows strong at a scale $\Lambda\sim 10^{-3}$ eV. We focus on the inflationary aspects of the model. Inflation occurs with a Coleman-Weinberg potential at a low scale, down to $\sim 6\times 10^5\gev$, being compatible with observational data.

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