Inflation and Dark Energy with a Single Superfield
arXiv:1412.2790 · doi:10.1088/1475-7516/2015/03/017
Abstract
We discuss the possibility to construct supergravity models with a single superfield describing inflation as well as the tiny cosmological constant . One could expect that the simplest way to do it is to study models with a supersymmetric Minkowski vacuum and then slightly uplift them. However, due to the recently proven no-go theorem, such a tiny uplifting cannot be achieved by a small modification of the parameters of the theory. We illustrate this general result by investigation of models with a single chiral superfield recently proposed by Ketov and Terada. We show that the addition of a small constant or a linear term to the superpotential of a model with a stable supersymmetric Minkowski vacuum converts it to an AdS vacuum, which results in a rapid cosmological collapse. One can avoid this problem and uplift a supersymmetric Minkowski vacuum to a dS vacuum with without violating the no-go theorem by making these extra terms large enough. However, we show that this leads to a strong supersymmetry breaking in the uplifted vacua.
15 pages, 7 figures. v2: refs added
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- Moduli Backreaction on Inflationary Attractors
- -term Multi-Field Inflation in Supergravity without Stabiliser Superfields
- Accelerating Universe in Terms of Hankel Function Index