Large-η constant-roll inflation is never an attractor

被引:43
|
作者
Morse, Michael J. P. [1 ]
Kinney, William H. [1 ]
机构
[1] Univ Buffalo, Dept Phys, Buffalo, NY 14260 USA
基金
美国国家科学基金会;
关键词
PHASE-TRANSITION; QUANTUM FLUCTUATIONS; UNIVERSE SCENARIO; DYNAMICS; FLATNESS; HORIZON;
D O I
10.1103/PhysRevD.97.123519
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Slow-roll solutions to inflationary potentials have been widely believed to be the only universal attractor. Over the past few years there has been growing interest in a new class of inflationary models known as constant-roll inflation. Constant-roll solutions are a generalization of "ultraslow roll" dynamics, where the first slow-roll parameter is small, but the second slow-roll parameter eta is larger than unity. In ultraslow roll inflation, the large-eta solution is a dynamical transient, relaxing exponentially to the attractor de Sitter solution. In the constant-roll generalization, recent papers have concluded that constant-roll inflation represents a new class of nonslow roll attractor solutions. In this paper we show that these attractor solutions are actually the usual slow-roll attractor, disguised by a parameter duality, and that the large-eta solutions, as in the case of ultraslow roll, represent a dynamical transient.
引用
收藏
页数:9
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