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Ellipsoidal Universe Can Solve The CMB Quadrupole Problem

L. Campanelli, P. Cea, L. Tedesco

Published 2006-06-12, updated 2006-09-22Version 2

The recent three-year WMAP data have confirmed the anomaly concerning the low quadrupole amplitude compared to the best-fit \Lambda CDM prediction. We show that, allowing the large-scale spatial geometry of our universe to be plane-symmetric with eccentricity at decoupling or order 10^{-2}, the quadrupole amplitude can be drastically reduced without affecting higher multipoles of the angular power spectrum of the temperature anisotropy.

Comments: 4 pages, 2 figures, minor changes, reference added, to appear in Phys. Rev. Lett
Journal: Phys.Rev.Lett.97:131302,2006; Erratum-ibid.97:209903,2006
Categories: astro-ph, gr-qc, hep-ph, hep-th
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