English

Multipole invariants and non-Gaussianity

Astrophysics 2009-11-10 v2

Abstract

We propose a framework for separating the information contained in the CMB multipoles, ama_{\ell m}, into its algebraically independent components. Thus we cleanly separate information pertaining to the power spectrum, non-Gaussianity and preferred axis effects. The formalism builds upon the recently proposed multipole vectors (Copi, Huterer & Starkman 2003; Schwarz & al 2004; Katz & Weeks 2004), and we elucidate a few features regarding these vectors, namely their lack of statistical independence for a Gaussian random process. In a few cases we explicitly relate our proposed invariants to components of the nn-point correlation function (power spectrum, bispectrum). We find the invariants' distributions using a mixture of analytical and numerical methods. We also evaluate them for the co-added WMAP first year map.

Keywords

Cite

@article{arxiv.astro-ph/0407081,
  title  = {Multipole invariants and non-Gaussianity},
  author = {Kate Land and Joao Magueijo},
  journal= {arXiv preprint arXiv:astro-ph/0407081},
  year   = {2009}
}
R2 v1 2026-07-22T08:39:57.670Z