Generalized G-Inflation - Inflation with the Most General Second-Order Field Equations

被引:1055
作者
Kobayashi, Tsutomu [1 ,2 ]
Yamaguchi, Masahide [3 ]
Yokoyama, Jun'ichi [4 ,5 ]
机构
[1] Kyoto Univ, Hakubi Ctr, Kyoto 6068302, Japan
[2] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
[3] Tokyo Inst Technol, Dept Phys, Tokyo 1528551, Japan
[4] Univ Tokyo, Grad Sch Sci, Res Ctr Early Universe RESCEU, Tokyo 1130033, Japan
[5] Univ Tokyo, IPMU, Kashiwa, Chiba 2778568, Japan
来源
PROGRESS OF THEORETICAL PHYSICS | 2011年 / 126卷 / 03期
关键词
NONLINEAR SUPERHORIZON PERTURBATIONS; GRADIENT EXPANSION APPROACH; CHAOTIC INFLATION; PHASE-TRANSITION; K-INFLATION; COSMOLOGY; UNIVERSE; SINGULARITY; FLATNESS; HORIZON;
D O I
10.1143/PTP.126.511
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study generalized Galileons as a framework to develop the most general single-field inflation models ever, Generalized G-inflation, containing yet further generalization of G-inflation, as well as previous examples such as k-inflation, extended inflation, and new Higgs inflation as special cases. We investigate the background and perturbation evolution in this model, calculating the most general quadratic actions for tensor and scalar cosmological perturbations to give the stability criteria and the power spectra of primordial fluctuations. It is pointed out in the Appendix that the Horndeski theory and the generalized Galileons are equivalent. In particular, even the non-minimal coupling to the Gauss-Bonnet term is included in the generalized Galileons in a non-trivial manner.
引用
收藏
页码:511 / 529
页数:19
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