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Phys. Rev. D 74, 021301(R) (2006) [5 pages]

Statistical isotropy of CMB polarization maps

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Soumen Basak1, Amir Hajian1,2,3, and Tarun Souradeep1
1Inter-University Centre for Astronomy and Astrophysics, Ganeshkhind, Post Bag 4, Pune-411007, India
2Department of Physics, Jadwin Hall, Princeton University, PO Box 708, Princeton, New Jersey 08542, USA
3Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, New Jersey 08544, USA

Received 22 March 2006; published 13 July 2006

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. The 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 3 yr data. As a demonstration we show that for E-polarization this test can detect the breakdown of statistical isotropy due to polarized synchrotron foreground.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.74.021301
DOI:
10.1103/PhysRevD.74.021301
PACS:
98.70.Vc