Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 5, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2013/05/011
Keywords
inflation; non-gaussianity; cosmological perturbation theory
Funding
- Lancaster-Manchester-Sheffield Consortium for Fundamental Physics under STFC [ST/J00418/1]
- European Research and Training Network (RTN) grant [UNILHC23792]
- CPAN [CSD2007-00042]
- MICINN [FIS2010-17395]
- Academy of Finland [131454]
- STFC [ST/J000418/1, ST/G00045X/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/G00045X/1, ST/J000418/1] Funding Source: researchfish
Ask authors/readers for more resources
The inflaton might be coupled to a gauge field through a term f(2)(phi)F mu nu F mu nu. If f proportional to a(-2) where a(t) is the scale factor, the perturbation delta W of the gauge field generates a potentially observable statistically anisotropic contribution to the primordial curvature perturbation during slow-roll inflation. The spectrum and bispectrum of this contribution have been calculated using the in-in formalism of quantum field theory. We give a simpler and more complete calculation using only the classical perturbations. The results suggest that either the entire curvature perturbation zeta (both the statistically isotropic and anisotropic parts) is generated during slow-roll inflation, or else it is generated afterwards.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available