arXiv · hep-th/9210114
Natural Supergravity Inflation
Abstract
We show that a single uncharged chiral superfield, canonically coupled to \mbox{$N=1$} supergravity with vanishing superpotential, naturally drives inflation in the early universe for a class of simple Kahler potentials. Inflation occurs due to the one-loop generation of a Kahler anomaly proportional to $\R^2$. The coefficient of this $\R^2$ term is of the correct magnitude to describe all aspects of an inflationary cosmology, including sufficient amplitude perturbations and reheating. Higher order terms proportional to $\R^n$ for $n \geq 3$ are naturally suppressed relative to the $\R^2$ term and, hence, do not destabilize the theory.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Gabriel Lopes Cardoso, Burt A. Ovrut. 1992-10-21. Natural Supergravity Inflation. https://doi.org/10.1016/0370-2693(93)91823-6
Cite the original work for its findings. Save a collection to share your selection of sources.