4.6 Article

Planck-suppressed operators

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2014/01/033

Keywords

inflation; non-gaussianity

Funding

  1. European Research Council (ERC STG grant) [279617]
  2. Stanford ITP
  3. U.S. Department of Energy [DE-AC02-76SF00515]
  4. NSF [PHY-0757868]

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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.

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