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2026 2

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Stochastic inflation from a non-equilibrium renormalization group

hep-th · 2026-05-11 · conditional · novelty 7.0

Stochastic inflation is the leading infrared limit of a coarse-grained Schwinger–Keldysh effective theory, and the same Fokker–Planck dynamics follows from a Polchinski-type renormalization-group flow for the reduced density matrix.

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