Modulated reheating by a curvaton

被引:9
|
作者
Choi, Ki-Young [1 ,2 ]
Seto, Osamu [3 ]
机构
[1] Asia Pacific Ctr Theoret Phys, Pohang 790784, Gyeongbuk, South Korea
[2] POSTECH, Dept Phys, Pohang 790784, Gyeongbuk, South Korea
[3] Hokkai Gakuen Univ, Dept Life Sci & Technol, Sapporo, Hokkaido 0628605, Japan
基金
新加坡国家研究基金会;
关键词
INFLATIONARY UNIVERSE SCENARIO; NON-GAUSSIANITY; PHASE-TRANSITION; PERTURBATIONS; DYNAMICS; FLATNESS; HORIZON;
D O I
10.1103/PhysRevD.85.123528
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
There might be a light scalar field during inflation which is not responsible for the accelerating inflationary expansion. Then, its quantum fluctuation is stretched during inflation. This scalar field could be a curvaton, if it decays at a late time. In addition, if the inflaton decay rate depends on the light scalar field expectation value by interactions between them, density perturbations could be generated by the quantum fluctuation of the light field when the inflaton decays. This is a modulated reheating mechanism. We study curvature perturbation in models where a light scalar field does not only play a role of curvaton but also induce modulated reheating at the inflaton decay. We calculate the nonlinearity parameters as well as the scalar spectral index and the tensor-to-scalar ratio. We find that there is a parameter region where nonlinearity parameters are also significantly enhanced by the cancellation between the modulated effect and the curvaton contribution. For the simple quadratic potential model of both inflaton and curvaton, both tensor-to-scalar ratio and nonlinearity parameters could be simultaneously large.
引用
收藏
页数:13
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