Deviations from Gaussian White Noise in Stochastic Inflation
Zahra Ahmadi, Mahdiyar Noorbala

TL;DR
This paper investigates how relaxing common assumptions in stochastic inflation affects the noise's character, showing that deviations from ideal conditions can produce colored, non-stationary, and non-Gaussian noise.
Contribution
It demonstrates how deviations from de Sitter background, window functions, and initial states modify the noise properties in stochastic inflation, including the emergence of colored and non-Gaussian noise.
Findings
Deviations from de Sitter background maintain white noise with time-dependent amplitude.
Non-Heaviside window functions or non-Bunch-Davies initial states can produce colored noise.
Non-Gaussian noise arises when the initial state deviates from Bunch-Davies vacuum.
Abstract
Stochastic inflation is widely used as a framework to study scalar field perturbations on an inflationary spacetime in a classical manner. In Starobinsky's seminal work and most of the subsequent literature, stochastic inflation is driven by a white noise. This is a consequence of a number of assumptions about the background metric, the window function, and the initial state. Given that noise is the central object in this approach, it is worthwhile to investigate how the noise is modified upon relaxing some of these assumptions. We show that while deviation from an exact de Sitter background maintains the white character of the noise (only with a time-dependent amplitude), deviation from the Heaviside window function or the Bunch-Davies initial state can produce colored noise. We calculate the power spectrum and the memory of the noise for a toy model with a piecewise linear window…
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Taxonomy
TopicsCosmology and Gravitation Theories · Stochastic processes and financial applications · Black Holes and Theoretical Physics
