English

Grand Unified Inflation Confronts WMAP

Astrophysics 2011-05-12 v2 High Energy Physics - Phenomenology

Abstract

In a class of realistic four and five dimensional supersymmetric grand unified models, the scalar spectral index is found to be ns=0.98(±0.01)n_s=0.98 (\pm 0.01), in excellent agreement with the values determined by several previous experiments and most recently by the Wilkinson Microwave Anisotropy Probe (WMAP). The models predict dns/dlnk103dn_s/d{\rm ln}k\sim 10^{-3} and a negligible tensor-to-scalar ratio r108r\sim 10^{-8}. A new five dimensional supersymmetric SO(10) model along these is presented in which inflation is associated with the breaking of SO(10) to SU(5) at scale MM, with δT/T(M/MPlanck)2\delta T/T\propto (M/M_{\rm Planck})^2, so that M1016M\simeq 10^{16} GeV. The inflaton decay leads to the observed baryon asymmetry via leptogenesis. We also discuss how the monopole problem is solved without the use of non-renormalizable terms.

Keywords

Cite

@article{arxiv.astro-ph/0302504,
  title  = {Grand Unified Inflation Confronts WMAP},
  author = {Bumseok Kyae and Qaisar Shafi},
  journal= {arXiv preprint arXiv:astro-ph/0302504},
  year   = {2011}
}

Comments

A new resolution of the monopole problem proposed. 1+9 pages

R2 v1 2026-07-22T08:20:48.846Z