Wess-Zumino Inflation in Light of Planck
Abstract
We discuss cosmological inflation in the minimal Wess-Zumino model with a single massive chiral supermultiplet. With suitable parameters and assuming a plausible initial condition at the start of the inflationary epoch, the model can yield scalar perturbations in the Cosmic Microwave Background (CMB) of the correct strength with a spectral index n_s ~ 0.96 and a tensor-to-scalar perturbation ratio r < 0.1, consistent with the Planck CMB data. We also discuss the possibility of topological inflation within the Wess-Zumino model, and the possibility of combining it with a seesaw model for neutrino masses. This would violate R-parity, but at such a low rate that the lightest supersymmetric particle would have a lifetime long enough to constitute the astrophysical cold dark matter.
Keywords
Cite
@article{arxiv.1303.6253,
title = {Wess-Zumino Inflation in Light of Planck},
author = {Djuna Croon and John Ellis and Nick E. Mavromatos},
journal= {arXiv preprint arXiv:1303.6253},
year = {2013}
}
Comments
11 pages, 3 figures