Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit
arXiv:astro-ph/9612202 · doi:10.1103/PhysRevD.55.R4516
Abstract
We present an analysis of CMB anisotropies induced by global scalar fields in the large N limit. In this limit, the CMB anisotropy spectrum can be determined without cumbersome 3D simulations. We determine the source functions and their unequal time correlation functions and show that they are quite similar to the corresponding functions in the texture model. This leads us to the conclusion that the large N limit provides a 'cheap approximation' to the texture model of structure formation.
11 pages Latex, 5 postscript figures included
Cited by in corpus (19)
- Measuring the dark side (with weak lensing)
- Cosmic Structure Formation with Topological Defects
- Metric preheating and limitations of linearized gravity
- Cosmic Microwave Background Anisotropies from Scaling Seeds: Global Defect Models
- Gravitational waves from self-ordering scalar fields
- Dark Energy in Practice
- Constraining topological defects with temperature and polarization anisotropies
- Skewness as a probe of non-Gaussian initial conditions
- Microwave Background Anisotropies from Scaling Seed Perturbations
- Level Set Method for the Evolution of Defect and Brane Networks
- Non-Gaussianity from Self-Ordering Scalar Fields
- Cosmological Evolution of Global Monopoles
- Cosmic Microwave Background Anisotropies from Scaling Seeds: Fit to Observational Data
- Scaling property and peculiar velocity of global monopoles
- Cosmic Microwave Background temperature and polarization anisotropies from the large-N limit of global defects
- The statistical physics of cosmological networks of string loops
- Dynamics of Symmetry Breaking in FRW Cosmologies: Emergence of Scaling
- Non-Equilibrium Large N Yukawa Dynamics: marching through the Landau pole
- Weak lensing from self-ordering scalar fields