Modulated curvaton decay

被引:13
作者
Assadullahi, Hooshyar [1 ,2 ]
Firouzjahi, Hassan [3 ]
Namjoo, Mohammad Hossein [4 ,5 ]
Wands, David [1 ]
机构
[1] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[2] Univ Portsmouth, Sch Earth & Environm Sci, Portsmouth PO1 3QL, Hants, England
[3] Inst Res Fundamental Sci IPM, Sch Astron, Tehran, Iran
[4] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[5] Inst Res Fundamental Sci IPM, Sch Phys, Tehran, Iran
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2013年 / 03期
关键词
inflation; non-gaussianity; NON-GAUSSIANITY; PERTURBATIONS; INFLATION; SCENARIO;
D O I
10.1088/1475-7516/2013/03/041
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study primordial density perturbations generated by the late decay of a curvaton field whose decay rate may be modulated by the local value of another isocurvature field, analogous to models of modulated reheating at the end of inflation. We calculate the primordial density perturbation and its local-type non-Gaussianity using the sudden-decay approximation for the curvaton field, recovering standard curvaton and modulated reheating results as limiting cases. We verify the Suyama-Yamaguchi inequality between bispectrum and trispectrum parameters for the primordial density field generated by multiple field fluctuations, and find conditions for the bound to be saturated.
引用
收藏
页数:15
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