Chaotic Inflation with a Fractional Power-Law Potential in Strongly Coupled Gauge Theories
Keisuke Harigaya, Masahiro Ibe, Kai Schmitz, and Tsutomu T. Yanagida

TL;DR
This paper demonstrates that chaotic inflation models with fractional power-law potentials can be realized within strongly coupled supersymmetric gauge theories, linking the inflationary potential's form to gauge dynamics and explaining the inflation scale.
Contribution
It introduces a novel realization of fractional power-law inflation models using strongly coupled supersymmetric gauge theories, connecting gauge dynamics to inflationary potential origin.
Findings
Fractional power-law inflation models are viable and testable.
The inflation energy scale is generated by strong gauge dynamics.
The model explains the smallness of the inflation scale relative to Planck scale.
Abstract
Models of chaotic inflation with a fractional power-law potential are not only viable but also testable in the foreseeable future. We show that such models can be realized in simple strongly coupled supersymmetric gauge theories. In these models, the energy scale during inflation is dynamically generated by the dimensional transmutation due to the strong gauge dynamics. Therefore, such models not only explain the origin of the fractional power in the inflationary potential but also provide a reason why the energy scale of inflation is much smaller than the Planck scale.
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