Warm quintessential inflation

被引:43
|
作者
Dimopoulos, Konstantinos [1 ]
Donaldson-Wood, Leonora [1 ]
机构
[1] Univ Lancaster, Phys Dept, Consortium Fundamental Phys, Lancaster LA1 4YB, England
关键词
COSMOLOGICAL CONSTANT; UNIVERSE; DYNAMICS;
D O I
10.1016/j.physletb.2019.07.017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We introduce warm quintessential inflation and study it in the weak dissipative regime. We consider the original quintessential inflation model, which approximates quartic chaotic inflation at early times and thawing quartic inverse-power-law quintessence at present. We find that the model successfully accounts for both inflation and dark energy observations, while it naturally reheats the Universe, thereby overcoming a major problem of quintessential inflation model-building. (C) 2019 The Author(s). Published by Elsevier B.V.
引用
收藏
页码:26 / 31
页数:6
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