Abstract
We consider a higher-order term in the 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 . Instead it produces a nonzero value of . A combination of constraints leads to an allowed region in space. To produce the asymmetry with this term without a large value of we find that the isocurvature field needs to contribute less than the inflation towards the power spectrum of the curvature perturbation.
- Received 6 May 2015
DOI:https://doi.org/10.1103/PhysRevD.92.023505
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