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Phys. Rev. Lett. 100, 181301 (2008) [4 pages]

Evidence of Primordial Non-Gaussianity (fNL) in the Wilkinson Microwave Anisotropy Probe 3-Year Data at 2.8σ

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Amit P. S. Yadav1 and Benjamin D. Wandelt1,2
1Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, Illinois 61801, USA
2Department of Physics, University of Illinois at Urbana-Champaign, 1110 W. Green Street, Urbana, Illinois 61801, USA

Received 7 December 2007; revised 6 March 2008; published 7 May 2008

We present evidence for primordial non-Gaussianity of the local type (fNL) in the temperature anisotropy of the cosmic microwave background. Analyzing the bispectrum of the Wilkinson Microwave Anisotropy Probe 3-year data up to max⁡=750 we find 27<fNL<147 (95% C.L.). This amounts to a rejection of fNL=0 at 2.8σ, disfavoring canonical single-field slow-roll inflation. The signal is robust to variations in lmax⁡, frequency and masks. No known foreground, instrument systematic, or secondary anisotropy explains it. We explore the impact of several analysis choices on the quoted significance and find 2.5σ to be conservative.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.100.181301
DOI:
10.1103/PhysRevLett.100.181301
PACS:
98.70.Vc, 98.80.Es