English

Non-Minimal Inflation after WMAP3

Astrophysics 2008-12-25 v2

Abstract

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.

Cite

@article{arxiv.0710.0058,
  title  = {Non-Minimal Inflation after WMAP3},
  author = {Kourosh Nozari and S. Davood Sadatian},
  journal= {arXiv preprint arXiv:0710.0058},
  year   = {2008}
}

Comments

16 pages, 11 figures, 2 tables, Revised Version

R2 v1 2026-06-21T09:23:56.046Z