English

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 101610^{16} GeV. This implies a GUT symmetry breaking scale of similar magnitude, and proton lifetime of order 103410^{34}-103810^{38} years. In some SO(10) models with axion dark matter, the scalar leptoquark boson exchange leads to proton decay with a lifetime of order 103410^{34}-103510^{35} 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

R2 v1 2026-06-21T11:32:59.199Z