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Stochastic non de Sitter Inflation

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arxiv hep-th/9305159 v3 pith:4SLUH3TD submitted 1993-05-28 hep-th gr-qc

Stochastic non de Sitter Inflation

classification hep-th gr-qc
keywords inflationstochasticaboveapproachcorrespondingdrivingequationequations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We generalize the stochastic approach to quasi-power-law inflationary Universes,obtain the corresponding Langevin and Fokker-Planck equations for the scalar field driving inflation and find stationary solutions to the above FP equation.

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  1. Deviations from Gaussian White Noise in Stochastic Inflation

    gr-qc 2025-12 conditional novelty 6.0

    Relaxing the sharp cutoff or the Bunch-Davies initial state in stochastic inflation makes the noise colored, and relaxing the initial state also makes it non-Gaussian.