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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.
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页数:9
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