The effective field theory of inflation/dark energy and the Horndeski theory

Shinji Tsujikawa*

*この研究の対応する著者

研究成果: Article査読

56 被引用数 (Scopus)

抄録

The effective field theory (EFT) of cosmological perturbations is a useful framework to deal with the low-energy degrees of freedom present for inflation and dark energy.We review the EFT for modified gravitational theories by starting from the most general action in unitary gauge that involves the lapse function and the three-dimensional geometric scalar quantities appearing in the Arnowitt- Deser-Misner (ADM) formalism. Expanding the action up to quadratic order in the perturbations and imposing conditions for the elimination of spatial derivatives higher than second order, we obtain the Lagrangian of curvature perturbations and gravitational waves with a single scalar degree of freedom. The resulting second-order Lagrangian is exploited for computing the scalar and tensor power spectra generated during inflation. We also show that the most general scalartensor theory with second-order equations of motion—Horndeski theory—belongs to the action of our general EFT framework and that the background equations of motion in Horndeski theory can be conveniently expressed in terms of three EFT parameters. Finally we study the equations of matter density perturbations and the effective gravitational coupling for dark energy models based on Horndeski theory, to confront the models with the observations of large-scale structures and weak lensing.

本文言語English
ページ(範囲)97-136
ページ数40
ジャーナルLecture Notes in Physics
892
DOI
出版ステータスPublished - 2015
外部発表はい

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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