Inflection point inflation and dark energy in supergravity
Tie-Jun Gao, Zong-Kuan Guo

TL;DR
This paper presents a supergravity inflation model with an inflection point that aligns with Planck data and explains current cosmic acceleration through a non-SUSY de-Sitter vacuum resulting from post-inflation supersymmetry breaking.
Contribution
It introduces a supergravity-based inflection point inflation model that simultaneously accounts for cosmic inflation and dark energy within a unified framework.
Findings
Predicted scalar spectral index and tensor-to-scalar ratio match Planck 2015 results.
Supersymmetry is strongly broken after inflation, leading to a non-SUSY de-Sitter vacuum.
Model provides a consistent explanation for both early universe inflation and late-time acceleration.
Abstract
We consider an inflection point inflationary model in supergravity with a single chiral superfield and show that the predicted values of the scalar spectral index and tensor-to-scalar ratio are consistent with the Planck 2015 results. In this model supersymmetry is strongly broken after inflation, which results in a non-SUSY de-Sitter vacuum responsible for the recent accelerated expansion of the Universe.
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