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November 2015 Angular spectra for non-Gaussian isotropic fields
György Terdik
Braz. J. Probab. Stat. 29(4): 833-865 (November 2015). DOI: 10.1214/14-BJPS249

Abstract

Cosmic microwave background (CMB) Anisotropies is a subject of intensive research in recent years, and therefore it is necessary to develop suitable theory and methods for the analysis of isotropic fields on spheres. The main object of our paper is to show that the polyspectra can be given as the coefficients of the orthogonal expansion of cumulants of the field in terms of irreducible tensor products of spherical harmonics. We obtain necessary and sufficient conditions for isotropy of a non-Gaussian field and the conditions are stated in terms of higher order spectra (polyspectra). The relation between cumulants and spectra gives a new method of estimating spectra.

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György Terdik. "Angular spectra for non-Gaussian isotropic fields." Braz. J. Probab. Stat. 29 (4) 833 - 865, November 2015. https://doi.org/10.1214/14-BJPS249

Information

Received: 1 December 2013; Accepted: 1 May 2014; Published: November 2015
First available in Project Euclid: 17 September 2015

zbMATH: 1328.83219
MathSciNet: MR3397396
Digital Object Identifier: 10.1214/14-BJPS249

Rights: Copyright © 2015 Brazilian Statistical Association

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Vol.29 • No. 4 • November 2015
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