Inflation and non-minimal scalar-curvature coupling in gravity and supergravity
Sergei V. Ketov, Alexei A. Starobinsky

TL;DR
This paper explores the equivalence between inflationary models with non-minimal scalar-curvature coupling in gravity and supergravity, extending the correspondence to N=1 supergravity using curved superspace, highlighting implications for inflationary dynamics.
Contribution
It extends the known correspondence between non-minimal scalar-curvature coupled gravity and f(R) gravity to N=1 supergravity, using curved superspace techniques.
Findings
Establishes equivalence of inflationary potentials in different theories
Rewrites non-minimal supergravity coupling in minimal form
Highlights differences in post-inflationary dynamics
Abstract
Inflationary slow-roll dynamics in Einstein gravity with a non-minimal scalar-curvature coupling can be equivalent to that in the certain f(R) gravity theory. We review the correspondence and extend it to N=1 supergravity. The non-minimal coupling in supergravity is rewritten in terms of the standard (`minimal') N=1 matter-coupled supergravity by using curved superspace. The established equivalence between two different inflationary theories means the same inflaton scalar potential, and does not imply the same post-inflationary dynamics and reheating.
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