Published May 1, 2013
| Version v1
Journal article
The statistically anisotropic curvature perturbation generated by f2(φ)FμνFμν
Creators
- 1. Consortium for Fundamental Physics, Cosmology and Astroparticle Group, Department of Physics, Lancaster University, Lancaster LA1 4YB (United Kingdom)
- 2. CAFPE and Departamento de Física Teórica y del Cosmos, Universidad de Granada, Granada-18071 (Spain)
Description
The inflaton might be coupled to a gauge field through a term f2(φ)FμνFμν. If f∝a−2 where a(t) is the scale factor, the perturbation δW 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 ζ (both the statistically isotropic and anisotropic parts) is generated during slow-roll inflation, or else it is generated afterwards
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2013/05/011Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2013
- Journal Issue
- 05
- Journal Page Range
- p. 011
- ISSN
- 1475-7516
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45104223
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANISOTROPY; ASTROPHYSICS; INFLATIONARY UNIVERSE; INFLATONS; PERTURBATION THEORY; POTENTIALS; QUANTUM FIELD THEORY
- Descriptors DEC
- COSMOLOGICAL MODELS; ELEMENTARY PARTICLES; FIELD THEORIES; MATHEMATICAL MODELS; PHYSICS; POSTULATED PARTICLES