GW170817-compatible constant-roll Einstein-Gauss-Bonnet inflation and non-Gaussianities

被引:39
作者
Odintsov, S. D. [1 ,2 ]
Oikonomou, V. K. [3 ,4 ,5 ]
Fronimos, F. P. [3 ]
Venikoudis, S. A. [3 ]
机构
[1] ICREA, Passeig Luis Co 23, Barcelona 08010, Spain
[2] CSIC, IEEC, Inst Space Sci, C Can Magrans S-N, Barcelona 08193, Spain
[3] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki 54124, Greece
[4] Tomsk State Univ Control Syst & Radioelect TUSUR, Lab Theoret Cosmol, Tomsk 634050, Russia
[5] Tomsk State Pedag Univ, Tomsk 634061, Russia
来源
PHYSICS OF THE DARK UNIVERSE | 2020年 / 30卷
关键词
Einstein-Gauss-Bonnet theory; Non-Gaussianities; Inflation; Early-time era; DILATONIC BLACK-HOLES; DARK-MATTER; MODIFIED GRAVITY; COSMOLOGICAL SOLUTIONS;
D O I
10.1016/j.dark.2020.100718
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we investigate the inflationary phenomenology of an Einstein-Gauss-Bonnet theory compatible with the GW170817 event, by imposing the constant-roll evolution on the scalar field. We develop the constant-roll GW170817-compatible Einstein-Gauss-Bonnet formalism, and we calculate the slow-roll indices and the observational indices of inflation, for several models of interest. As we demonstrate, the phenomenological viability of the models we study is achieved for a wide range of the free parameters. In addition, for the same values of the free parameters that guarantee the inflationary phenomenological viability of the models, we also make predictions for the non-Gaussianities of the models, since the constant-roll evolution is known to enhance non-Gaussianities. As we show the non-Gaussianities are of the same order for the slow-roll and constant-roll case, and in fact in some cases, the amount of the non-Gaussianities is smaller in the constant-roll case. (c) 2020 Elsevier B.V. All rights reserved.
引用
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页数:10
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