Ellipsoidal Universe Induces Large Scale CMB Polarization

Abstract

We calculate the large scale polarization of the cosmic microwave background induced by the anisotropy of the spatial geometry of our universe. Assuming an eccentricity at decoupling of about $0.6410^{-2}$, we find $\hat{I}”T_{pol}/T_0\simeq 0.5310^{-6}$ quite close to the average level of polarization detected by the Wilkinson Microwave Anisotropy Probe.

revised version, 9 pages