4.6 Article

A manifestly covariant theory of multifield stochastic inflation in phase space: solving the discretisation ambiguity in stochastic inflation

Journal

Publisher

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2021/04/048

Keywords

inflation; physics of the early universe; cosmological perturbation theory; quantum field theory on curved space

Funding

  1. European Research Council under the European Union's Horizon 2020 research and innovation programme [758792]
  2. JSPS KAKENHI Grants [JP18J01992, JP19K14707]
  3. Region Ile-de-France

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This paper addresses the issues in stochastic inflation theory by using Stratonovich discretization satisfying general covariance and identifying the quantum nature of fluctuating fields leading to the existence of preferred frame defining independent stochastic noises. Physically equivalent Ito-Langevin equations are derived which are manifestly covariant and well suited for numerical computations.
Stochastic inflation is an effective theory describing the super-Hubble, coarse grained, scalar fields driving inflation, by a set of Langevin equations. We previously high lighted the difficulty of deriving a theory of stochastic inflation that is invariant under field redefinitions, and the link with the ambiguity of discretisation schemes defining stochastic differential equations. In this paper, we solve the issue of these inflationary stochastic anomalies by using the Stratonovich discretisation satisfying general covariance, and identifying that the quantum nature of the fluctuating fields entails the existence of a preferred frame defining independent stochastic noises. Moreover, we derive physically equivalent Ito-Langevin equations that are manifestly covariant and well suited for numerical computations. These equations are formulated in the general context of multifield inflation with curved field space, taking into account the coupling to gravity as well as the full phase space in the Hamiltonian language, but this resolution is also relevant in simpler single-field setups. We also develop a path-integral derivation of these equations, which solves conceptual issues of the heuristic approach made at the level of the classical equations of motion, and allows in principle to compute corrections to the stochastic formalism. Using the Schwinger-Keldysh formalism, we integrate out small-scale fluctuations, derive the influence action that describes their effects on the coarse-grained fields, and show how the resulting coarse-grained effective Hamiltonian action can be interpreted to derive Langevin equations with manifestly real noises. Although the corresponding dynamics is not rigorously Markovian, we show the covariant, phase-space Fokker-Planck equation for the Probability Density Function of fields and momenta when the Markovian approximation is relevant, and we give analytical approximations for the noises' amplitudes in multifield scenarios.

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