Resonant non-Gaussianity with equilateral properties

被引:3
作者
Gwyn, Rhiannon [1 ]
Rummel, Markus [2 ]
Westphal, Alexander [3 ]
机构
[1] AEI Max Planck Inst Gravitat Phys, D-14476 Potsdam, Germany
[2] Univ Hamburg, Inst Theoret Phys 2, D-22761 Hamburg, Germany
[3] Deutsch Elektronen Synchrotron DESY, Theory Grp, D-22603 Hamburg, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2013年 / 04期
基金
欧洲研究理事会;
关键词
inflation; non-gaussianity; axions; string theory and cosmology; POWER SPECTRUM; FLUCTUATIONS; TELESCOPE; UNIVERSE; SKY;
D O I
10.1088/1475-7516/2013/04/040
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the effect of superimposing multiple sources of resonant non-Gaussianity, which arise for instance in models of axion inflation. The resulting sum of oscillating shape contributions can be used to "Fourier synthesize" different non-oscillating shapes in the bispectrum. As an example we reproduce an approximately equilateral shape from the superposition of O(10) oscillatory contributions with resonant shape. This implies a possible degeneracy between the equilateral-type non-Gaussianity typical of models with non-canonical kinetic terms, such as DBI inflation, and an equilateral-type shape arising from a superposition of resonant-type contributions in theories with canonical kinetic terms. The absence of oscillations in the 2-point function together with the structure of resonant N-point functions give a constraint of f(NL) less than or similar to O(5) for equilateral non-Gaussianity with resonant origin, but this constraint can be avoided when additional U(1)s are involved in the breaking of the shift symmetry. We comment on the questions arising from possible embeddings of this idea in a string theory setting.
引用
收藏
页数:28
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