Testing the Gaussianity and Statistical Isotropy of the Universe
arXiv:1012.3744 · doi:10.1155/2010/697147
Abstract
The last few years have seen a surge in excitement about measurements of statistics of the primordial fluctuations beyond the power spectrum. New ideas for precision tests of Gaussianity and statistical isotropy in the data are developing simultaneously with proposals for a wide range of new theoretical possibilities. From both the observations and theory, it has become clear that there is a huge discovery potential from upcoming measurements. In this Special Issue of Advances in Astronomy we have collected articles that summarize the theoretical predictions for departures from Gaussianity or statistical isotropy from a variety of potential sources, together with the observational approaches to test these properties using the CMB or large-scale structure. We hope this collection provides an accessible entry point to these topics as they currently stand, indicating what direction future developments may take and demonstrating why these questions are so compelling. The Special Issue is available at http://www.hindawi.com/journals/aa/2010/si.gsiu.html, and individual articles are also available on the arXiv.
This is the editorial foreword which introduces the Special Issue on Statistical Isotropy and Gaussianity published in Advances in Astronomy. The issue contains fifteen review papers; all papers were peer-reviewed by a minimum of two referees. To read the Special Issue, please follow http://www.hindawi.com/journals/aa/2010/si.gsiu.html
Cited by in corpus (8)
- The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
- Exact Mapping between Tensor and Most General Scalar Power Spectra
- All sky CMB map from cosmic strings integrated Sachs-Wolfe effect
- Self-Calibration for 3-point Intrinsic Alignment Auto-Correlations in Weak Lensing Surveys
- Self-calibrating the gravitational shear-intrinsic ellipticity-intrinsic ellipticity (GII) cross-correlation
- Squeezed primordial bispectrum from general vacuum state
- Permutation invariant Gaussian 2-matrix models
- Scale and shape dependent non-Gaussianity in the presence of inflationary vector fields