This research derives stochastic equations for inflation involving higher-curvature gravity terms, revealing influences on scalar field dynamics.
We study stochastic inflation in the presence of higher-curvature terms non-minimally coupled to the inflaton. Focusing on quadratic curvature invariants, we single out the Gauss--Bonnet term which is known to avoid ghosts, while having non-trivial effects on the background and scalar mode evolution when coupled to the scalar field. Stochastic Klein--Gordon and Langevin equations are derived in the presence of the Gauss--Bonnet coupling, and their slow-roll and ultra-slow-roll limits are studied. By using first-passage time method, scalar power spectrum is computed in these limits. Stochastic evolution of a Gauss--Bonnet-coupled spectator field in de Sitter vacuum is also discussed.
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Aldabergenov et al. (2025) studied this question.
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