Revisiting the spectrum of a scalar field in an anisotropic universe
gr-qc, astro-ph.CO, hep-th
Submitted: 2012-11-06
Updated: 2012-11-06
Comments: 22pages, 1figure
Journal ref: Journal of the Korean Physical Society, 64, 1 2014, pp. 140
DOI: 10.3938/jkps.64.140
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Statistical Anisotropy from Anisotropic Inflation
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Non-Gaussianity as a Probe of the Physics of the Primordial Universe and the Astrophysics of the Low Redshift Universe
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Primordial Non-Gaussianities from Inflation Models
- Non-Gaussianity of quantum fields during inflation
- Local non-Gaussianity from inflation
- Inhomogeneous cosmological models: exact solutions and their applications
- Imprints of a Primordial Preferred Direction on the Microwave Background
- Primordial statistical anisotropy generated at the end of inflation
- Anisotropic non-Gaussianity from vector field perturbations
- Predictions from an anisotropic inflationary era
- Gravity Waves Signatures from Anisotropic pre-Inflation
- Instability of anisotropic cosmological solutions supported by vector fields
- Instability of the ACW model, and problems with massive vectors during inflation
- Ghost instabilities of cosmological models with vector fields nonminimally coupled to the curvature
- Vector theories in cosmology
- An analytic approach to perturbations from an initially anisotropic universe
- String or branelike solutions in four-dimensional Einstein gravity in the presence of cosmological constant
- Cylindrical Black Hole in General Relativity
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