Generating the cosmic microwave background power asymmetry with gNL

Zachary Kenton, David J. Mulryne, and Steven Thomas
Phys. Rev. D 92, 023505 – Published 6 July 2015

Abstract

We consider a higher-order term in the δN expansion for the cosmic microwave background power asymmetry generated by a superhorizon isocurvature field fluctuation. The term can generate the asymmetry without requiring a large value of fNL. Instead it produces a nonzero value of gNL. A combination of constraints leads to an allowed region in fNLgNL space. To produce the asymmetry with this term without a large value of fNL we find that the isocurvature field needs to contribute less than the inflation towards the power spectrum of the curvature perturbation.

  • Figure
  • Received 6 May 2015

DOI:https://doi.org/10.1103/PhysRevD.92.023505

© 2015 American Physical Society

Authors & Affiliations

Zachary Kenton*, David J. Mulryne, and Steven Thomas

  • School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, United Kingdom

  • *z.a.kenton@qmul.ac.uk
  • d.mulryne@qmul.ac.uk
  • s.thomas@qmul.ac.uk

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Issue

Vol. 92, Iss. 2 — 15 July 2015

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