Generating non-Gaussian maps with a given power spectrum and bispectrum
arXiv:astro-ph/0101512 · doi:10.1103/PhysRevD.63.103512
Abstract
We propose two methods for generating non-Gaussian maps with fixed power spectrum and bispectrum. The first makes use of a recently proposed rigorous, non-perturbative, Bayesian framework for generating non-Gaussian distributions. The second uses a simple superposition of Gaussian distributions. The former is best suited for generating mildly non-Gaussian maps, and we discuss in detail the limitations of this method. The latter is better suited for the opposite situation, i.e. generating strongly non-Gaussian maps. The ensembles produced are isotropic and the power spectrum can be jointly fixed; however we cannot set to zero all other higher order cumulants (an unavoidable mathematical obstruction). We briefly quantify the leakage into higher order moments present in our method. We finally present an implementation of our code within the HEALPIX package
22 pages submitted to PRD, astro-ph version only includes low resolution maps
Cited by in corpus (19)
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- General CMB and Primordial Bispectrum Estimation I: Mode Expansion, Map-Making and Measures of f_NL
- Algorithms for bispectra: forecasting, optimal analysis, and simulation
- High-Resolution Simulations of Cosmic Microwave Background non-Gaussian Maps in Spherical Coordinates
- Estimate of the Cosmological Bispectrum from the MAXIMA-1 Cosmic Microwave Background Map
- Simulation of non-Gaussian CMB maps
- The CMB temperature bispectrum induced by cosmic strings
- Multiple Methods for Estimating the Bispectrum of the Cosmic Microwave Background with Application to the MAXIMA Data
- Moment transport equations for the primordial curvature perturbation
- Numerical Simulation of Non-Gaussian Random Fields with Prescribed Correlation Structure
- Non-Gaussian gravitational clustering field statistics
- Estimating the bispectrum of the Very Small Array data
- Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
- Statistical nature of non-Gaussianity from cubic order primordial perturbations: CMB map simulations and genus statistic
- Non-perturbative
- Characterizing the spatial pattern of solar supergranulation using the bispectrum
- Generation of Arbitrarily Non-Gaussian Fields with a Set Correlation Structure
- Phenomenological aspects of dark energy dominated cosmologies
- Some characterizations of the spherical harmonics coefficients for isotropic random fields