New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data

被引:8
作者
Behbahani, Siavosh R. [1 ]
Mirbabayi, Mehrdad [2 ]
Senatore, Leonardo [3 ,4 ,5 ]
Smith, Kendrick M. [6 ]
机构
[1] Boston Univ, Dept Phys, Boston, MA 02215 USA
[2] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA
[3] Stanford Univ, Stanford Inst Theoret Phys, Stanford, CA 94306 USA
[4] SLAC, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA
[5] Stanford Univ, Menlo Pk, CA 94025 USA
[6] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
基金
美国国家科学基金会; 加拿大创新基金会; 加拿大自然科学与工程研究理事会;
关键词
inflation; non-gaussianity; PRIMORDIAL NON-GAUSSIANITY; ANISOTROPIES;
D O I
10.1088/1475-7516/2014/11/035
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Given the fantastic experimental effort, it is important to thoroughly explore the signature space of inflationary models. The fact that higher derivative operators do not renormalize lower derivative ones allows us to find a large class of technically natural single-clock inflationary models where, in the context of the Effective Field Theory of Inflation, the leading interactions have many derivatives. We systematically explore the 3-point function induced by these models and their overlap with the standard equilateral and orthogonal templates. We find that in order to satisfactorily cover the signature space of these models, two new additional templates need to be included. We then perform the optimal analysis of the WMAP 9-year data for the resulting four templates, finding that the overall significance of a non-zero signal is between 2-2.5 sigma, depending on the choice of parameter space, partially driven by the preference for nonzero f(NL)(orth) in WMAP9.
引用
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页数:31
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