Nonlinear perturbations of cosmological scalar fields with non-standard kinetic terms

We adopt a covariant formalism to derive exact evolution equations for nonlinear perturbations, in a universe dominated by two scalar fields. These scalar fields are characterized by non-canonical kinetic terms and an arbitrary field space metric, a situation typically encountered in inflationary mo...

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Published inJournal of cosmology and astroparticle physics Vol. 2009; no. 1; p. 012
Main Authors Renaux-Petel, Sébastien, Tasinato, Gianmassimo
Format Journal Article
LanguageEnglish
Published United States IOP Publishing 01.01.2009
Institute of Physics (IOP)
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Summary:We adopt a covariant formalism to derive exact evolution equations for nonlinear perturbations, in a universe dominated by two scalar fields. These scalar fields are characterized by non-canonical kinetic terms and an arbitrary field space metric, a situation typically encountered in inflationary models inspired by string theory. We decompose the nonlinear scalar perturbations into adiabatic and entropy modes, generalizing the definition adopted in the linear theory, and we derive the corresponding exact evolution equations. We also obtain a nonlinear generalization of the curvature perturbation on uniform density hypersurfaces, showing that on large scales it is sourced only by the nonlinear version of the entropy perturbation. We then expand these equations to second order in the perturbations, using a coordinate based formalism. Our results are relatively compact and elegant and enable one to identify the new effects coming from the non-canonical structure of the scalar fields Lagrangian. We also explain how to analyze, in our formalism, the interesting scenario of multi-field Dirac-Born-Infeld inflation.
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ISSN:1475-7516
1475-7508
1475-7516
DOI:10.1088/1475-7516/2009/01/012