4.6 Article

Modulation of the waterfall by a gauge field

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2013/01/031

Keywords

cosmological perturbation theory; inflation; non-gaussianity

Funding

  1. Lancaster-Manchester-Sheffield Consortium for Fundamental Physics under STFC [ST/J00418/1]
  2. European Research and Training Network (RTN) [UNILHC23792]
  3. MICINN [FIS2010-17395]
  4. [CPAN CSD2007-00042]
  5. Science and Technology Facilities Council [ST/G00045X/1, ST/J000418/1] Funding Source: researchfish
  6. STFC [ST/J000418/1, ST/G00045X/1] Funding Source: UKRI

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We present the first complete calculation of the curvature perturbation generated during the hybrid inflation waterfall, caused by the coupling of the waterfall field to a gauge field A whose kinetic function f(2) depends on the inflaton field. We impose an upper bound on the field W equivalent to f A which ensures that it has a negligible effect before the waterfall. We confirm the claim of Soda and Yokoyama, that the perturbation delta W generates a statistically anisotropic spectrum and bispectrum, which could easily be observable. We also discover a new phenomenon, whereby the time-dependent 'varyon' field W causes the inflaton contribution to vary during the waterfall. The varyon mechanism might be implemented also with a scalar field and might not involve the waterfall.

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