Non-Minimal Inflation after WMAP3

Details Non-Minimal Inflation after WMAP3 Non-Minimal Inflation after WMAP3

2007-09-29

arxiv.org/abs/0710.0058v2

Mod.Phys.Lett.A23:2933-2945,2008

Astronomy and Astrophysics

Astrophysics

16 pages, 11 figures, 2 tables, Revised Version

Scientific paper

10.1142/S0217732308026698

The Wilkinson Microwave Anisotropy Probe (WMAP) three year results are used to constraint non-minimal inflation models. Two different non-minimally coupled scalar field potentials are considered to calculate corresponding slow-roll parameters of non-minimal inflation. The results of numerical analysis of parameter space are compared with WMAP3 data to find appropriate new constraints on the values of the non-minimal coupling. A detailed comparison of our results with previous studies reveals the present status of the non-minimal inflation model after WMAP3.

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