Friction in Stochastic Inflation
Baptiste Blachier, Christophe Ringeval

TL;DR
This paper derives an exact probability distribution for curvature fluctuations in stochastic inflation with friction, revealing exponential tails and differences between forward and reverse approaches, especially in eternal inflation scenarios.
Contribution
It introduces a time-reversed stochastic inflation framework with friction, providing exact solutions and comparing them to traditional methods, highlighting new insights into inflationary fluctuations.
Findings
Exponential decay in curvature fluctuation tails contrasts with Levy-like power laws.
Time-reversed formalism yields Gaussian tails in the classical limit.
Negative drift leads to eternal inflation with finite curvature distribution.
Abstract
We solve time-reversed stochastic inflation in the semi-infinite flat potential with a constant drift term and derive an exact expression for the probability distribution of the curvature fluctuations. It exhibits exponential decaying tails which contrast to the Levy-like power law behaviour encountered without friction. Such a non-vanishing drift acts as a regulator for the conventional ``forward'' stochastic -formalism, which is otherwise ill-defined in the unbounded and flat potentials typical of plateau models of inflation. This setup therefore allows us to compare the curvature distribution derived from both approaches, reverse and forward in time. Up to similar exponential tails, we find quantitative differences. In particular, in the classical-like limit of very large drift, the tails become Gaussian but only in the time-reversed picture. As a toy model of eternal…
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Taxonomy
TopicsStochastic processes and financial applications · Cosmology and Gravitation Theories · Geometry and complex manifolds
