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Statistical Isotropy of CMB Polarization Maps

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arxiv astro-ph/0603406 v2 pith:WBJYFT36 submitted 2006-03-16 astro-ph hep-th

classification astro-phhep-th
keywords mapspolarizationstatisticalisotropyforegroundpolarizedanisotropyapplication
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We formulate statistical isotropy of CMB anisotropy maps in its most general form. We also present a fast and orientation independent statistical method to determine deviations from statistical isotropy in CMB polarization maps. Importance of having statistical tests of departures from SI for CMB polarization maps lies not only in interesting theoretical motivations but also in testing cleaned CMB polarization maps for observational artifacts such as residuals from polarized foreground emission. We propose a generalization of the Bipolar Power Spectrum (BiPS) to polarization maps. Application to the observed CMB polarization maps will be soon possible after the release of WMAP three year data. As a demonstration we show that for E-polarization this test can detect breakdown of statistical isotropy due to polarized synchrotron foreground.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. CMB sky for an off-center observer in a local void I: framework for forecasts

    astro-ph.CO 2019-08 conditional novelty 6.0 of 10

    An off-center observer in an LTB void would see off-diagonal CMB correlations; the paper develops a Fisher forecast framework and finds S/N > 10 for two illustrative void models with Planck.

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