A new parameter in attractor single-field inflation

被引:4
作者
Gong, Jinn-Ouk [1 ,2 ]
Sasaki, Misao [3 ]
机构
[1] Asia Pacific Ctr Theoret Phys, Pohang 790784, South Korea
[2] Postech, Dept Phys, Pohang 790784, South Korea
[3] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
基金
新加坡国家研究基金会;
关键词
HORIZON; PERTURBATIONS; FLATNESS; UNIVERSE;
D O I
10.1016/j.physletb.2015.06.023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We revisit the notion of slow-roll in the context of general single-field inflation. As a generalization of slow-roll dynamics, we consider an inflaton phi in an attractor phase where the time derivative of phi is determined by a function of phi, phi = phi(phi). In other words, we consider the case when the number of e-folds N counted backward in time from the end of inflation is solely a function of phi, N = N(phi). In this case, it is found that we need a new independent parameter to properly describe the dynamics of the inflaton field in general, in addition to the standard parameters conventionally denoted by epsilon, eta, c(s)(2) and s. Two illustrative examples are presented to discuss the non-slow-roll dynamics of the inflaton field consistent with observations. (C) 2015 The Authors. Published by Elsevier B.V.
引用
收藏
页码:390 / 394
页数:5
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