English

Covariant second-order perturbations in generalized two-field inflation

Cosmology and Nongalactic Astrophysics 2014-07-28 v2 High Energy Physics - Theory

Abstract

We examine the covariant properties of generalized models of two-field inflation, with non-canonical kinetic terms and a possibly non-trivial field metric. We demonstrate that kinetic-term derivatives and covariant field derivatives do commute in a proper covariant framework, which was not realized before in the literature. We also define a set of generalized slow-roll parameters, using a unified notation. Within this framework, we study the most general class of models that allows for well-defined adiabatic and entropic sound speeds, which we identify as the models with parallel momentum and field velocity vectors. For these models we write the exact cubic action in terms of the adiabatic and isocurvature perturbations. We thus provide the tool to calculate the exact non-Gaussianity beyond slow-roll and at any scale for these generalized models. We illustrate our general results by considering their long-wavelength limit, as well as with the example of two-field DBI inflation.

Keywords

Cite

@article{arxiv.1312.6139,
  title  = {Covariant second-order perturbations in generalized two-field inflation},
  author = {Eleftheria Tzavara and Shuntaro Mizuno and Bartjan van Tent},
  journal= {arXiv preprint arXiv:1312.6139},
  year   = {2014}
}

Comments

39 pages, no figures, minor changes and clarifications

R2 v1 2026-06-22T02:33:02.867Z