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We describe a simple way of incorporating fluctuations of the Hubble scale during the horizon exit of scalar perturbations into the delta N formalism.
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A. A. Starobinsky, “Stochastic de Sitter (Inflationary) Stage in the Early Universe,” In *De Vega, H.j. ( Ed.), Sanchez, N. ( Ed.): Field Theory, Quantum Gravity and Strings*, 107-126
Cited in the paper.