Non-Gaussianity from symmetry

被引:47
|
作者
Suyama, Teruaki [1 ]
Takahashi, Fuminobu [2 ]
机构
[1] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[2] Univ Tokyo, Inst Phys & Math Universe, Chiba 2778568, Japan
关键词
cosmological perturbation theory; inflation; physics of the early universe;
D O I
10.1088/1475-7516/2008/09/007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We point out that a light scalar field fluctuating around a symmetry-enhanced point can generate large non-Gaussianity in density fluctuations. We name such a particle an 'ungaussiton', a scalar field dominantly produced by the quantum fluctuations, generating sizable non-Gaussianity in the density fluctuations. We derive a consistency relation between the bispectrum and the trispectrum, tau NL similar to 10(3) center dot f(NL)(4/3), which can be extended to arbitrarily high order correlation functions. If such a relation is confirmed by future observations, it will strongly support this mechanism.
引用
收藏
页数:18
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