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Non-linear perturbations in multiple-field inflation

G. I. Rigopoulos·E. P. S. Shellard·B. J. W. van Tent
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Abstract

We develop a non-linear framework for describing long-wavelength perturbations in multiple-field inflation. The basic variables describing inhomogeneities are defined in a non-perturbative manner, are invariant under changes of time slicing on large scales and include both matter and metric perturbations. They are combinations of spatial gradients generalising the gauge-invariant variables of linear theory. Dynamical equations are derived and supplemented with stochastic source terms which provide the long-wavelength initial conditions determined from short-wavelength modes. Solutions can be readily obtained via numerical simulations or analytic perturbative expansions. The latter are much simpler than the usual second-order perturbation theory. Applications are given in a companion paper.

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G. I. Rigopoulos, E. P. S. Shellard, B. J. W. van Tent. 2006-05-05. Non-linear perturbations in multiple-field inflation. https://doi.org/10.1103/physrevd.73.083521

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