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arxiv: 2506.21423 · v2 · submitted 2025-06-26 · 🌀 gr-qc · astro-ph.CO· hep-th

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Towards Stochastic Inflation in Higher-Curvature Gravity

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classification 🌀 gr-qc astro-ph.COhep-th
keywords stochasticscalarcoupledevolutionfieldgauss-bonnethigher-curvatureinflation
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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 and PBH mass fraction are estimated in these limits. Stochastic evolution of a Gauss-Bonnet-coupled spectator field in de Sitter vacuum is also discussed.

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Cited by 1 Pith paper

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