Fast computation of first-order feature-bispectrum corrections

Peter Adshead and Wayne Hu
Phys. Rev. D 85, 103531 – Published 29 May 2012

Abstract

Features in the inflaton potential that are traversed in much less than an e-fold of the expansion can produce observably large non-Gaussianity. In these models first-order corrections to the curvature mode function evolution induce effects at second order in the slow-roll parameters that are generically greater than 10% and can reach order unity for order unity power spectrum features. From a complete first-order expression in generalized slow roll, we devise a computationally efficient method that is as simple to evaluate as the leading-order one and implements consistency relations in a controlled fashion. This expression matches direct numerical computation for step potential models of the dominant bispectrum configurations to better than 1% when features are small and 10% when features are order unity.

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  • Received 9 March 2012

DOI:https://doi.org/10.1103/PhysRevD.85.103531

© 2012 American Physical Society

Authors & Affiliations

Peter Adshead1 and Wayne Hu1,2

  • 1Kavli Institute for Cosmological Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
  • 2Department of Astronomy & Astrophysics, University of Chicago, Chicago Illinois 60637, USA

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Issue

Vol. 85, Iss. 10 — 15 May 2012

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