GUT Inflation and Proton Decay after WMAP5
High Energy Physics - Phenomenology
2010-04-15 v1 Astrophysics
Abstract
We employ Coleman-Weinberg and Higgs potentials to implement inflation in non-supersymmetric grand unified theories (GUTs) such as SU(5) and SO(10). To realize a scalar spectral index close to 0.96, as indicated by the most recent WMAP 5-year anlaysis, the energy scale of observable inflation turns out to be of order GeV. This implies a GUT symmetry breaking scale of similar magnitude, and proton lifetime of order - years. In some SO(10) models with axion dark matter, the scalar leptoquark boson exchange leads to proton decay with a lifetime of order - years.
Keywords
Cite
@article{arxiv.0810.3625,
title = {GUT Inflation and Proton Decay after WMAP5},
author = {Mansoor Ur Rehman and Qaisar Shafi and Joshua R. Wickman},
journal= {arXiv preprint arXiv:0810.3625},
year = {2010}
}
Comments
15 pages, 4 figures