Stochastic inflaton wave equation from an expanding environment
arXiv:2001.07268 · doi:10.1140/epjc/s10052-020-7877-y
Abstract
We discuss the inflaton in an environment of scalar fields on flat and curved manifolds. We average over the environmental fields . We study a contribution of superhorizon as well as subhorizon modes . As a result we obtain a stochastic wave equation with a friction and noise. We show that in the subhorizon regime in field theory a finite number of fields is sufficient to produce a friction and diffusion owing to the infinite number of degrees of freedom corresponding to different in . We investigate the slow roll and the Markovian approximaions to the stochastic wave equation. A determination of the metric from the stochastic Einstein-Klein-Gordon equations is briefly discussed,
arXiv commentminor changes, 10 pages
References in corpus (13)
- Towards the Theory of Reheating After Inflation
- Inflation Dynamics and Reheating
- Semiclassicality and Decoherence of Cosmological Perturbations
- Thermally Induced Density Perturbations in the Inflation Era
- Inflation and squeezed quantum states
- Warm Inflation and its Microphysical Basis
- Warm Inflation in the Adiabatic Regime- a Model, an Existence Proof for Inflationary Dynamics in Quantum Field Theory
- Correlation Functions in Stochastic Inflation
- Thermal Properties of an Inflationary Universe
- Generation of fluctuations during inflation: comparison of stochastic and field-theoretic approaches
- Stabilization of Starobinsky-Vilenkin stochastic inflation by an environmental noise
- Stochastic wave equation with thermal noise in an expanding universe
- Slow-roll versus stochastic slow-roll inflation