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Planck-suppressed operators

delete2014-01-23
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A
Assassi, Valentin *
B
Baumann, Daniel
D
Daniel Green
L
Liam McAllister
DOI:10.1088/1475-7516/2014/01/033delete
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Abstract

Abstract

En 中文
We show that the recent Planck limits on primordial non-Gaussianity impose strong constraints on light hidden sector fields coupled to the inflaton via operators suppressed by a high mass scale A. We study a simple effective field theory in which a hidden sector field is coupled to a shift-symmetric inflaton via arbitrary operators up to dimension five. Self-interactions in the hidden sector lead to non-Gaussianity in the curvature perturbations. To be consistent with the Planck limit on local non-Gaussianity, the coupling to any hidden sector with light fields and natural cubic couplings must be suppressed by a very high scale Lambda > 10(5)H. Even if the hidden sector has Gaussian correlations, nonlinearities in the mixing with the inflaton still lead to non-Gaussian curvature perturbations. In this case, the non-Gaussianity is of the equilateral or orthogonal type, and the Planck data requires Lambda > 10(2)H.
Keywords:
inflation
non-gaussianity
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Journal

Journal of Cosmology and Astroparticle Physics cover
Journal of Cosmology and Astroparticle Physics
IF:
5.9
Papers:
1.3W
Citations:
4.7W

Organization

S
Stanford University
Scholars:
9.6W
Papers: 8.2W
Citations: 17.0W
U
University of Cambridge
Scholars:
7.7W
Papers: 7.1W
Citations: 13.7W
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