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Phys. Rev. Lett. 96, 221302 (2006) [4 pages]

Searching for CPT Violation with Cosmic Microwave Background Data from WMAP and BOOMERANG

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Bo Feng1,2, Mingzhe Li3, Jun-Qing Xia4, Xuelei Chen1, and Xinmin Zhang4
1National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China
2Research Center for the Early Universe (RESCEU), Graduate School of Science, University of Tokyo, Tokyo 113-0033, Japan
3Institut für Theoretische Physik, Philosophenweg 16, 69120 Heidelberg, Germany
4Institute of High Energy Physics, Chinese Academy of Science, P.O. Box 918-4, Beijing 100049, People’s Republic of China

Received 23 January 2006; revised 16 May 2006; published 7 June 2006

See accompanying Physics Focus

We search for signatures of Lorentz and CPT violations in the cosmic microwave background (CMB) temperature and polarization anisotropies by using the Wilkinson Microwave Anisotropy Probe (WMAP) and the 2003 flight of BOOMERANG (B03) data. We note that if the Lorentz and CPT symmetries are broken by a Chern-Simons term in the effective Lagrangian, which couples the dual electromagnetic field strength tensor to an external four-vector, the polarization vectors of propagating CMB photons will get rotated. Using the WMAP data alone, one could put an interesting constraint on the size of such a term. Combined with the B03 data, we found that a nonzero rotation angle of the photons is mildly favored: Δα=-6.0+4.0/-4.0+3.9/-3.7  deg⁡(1,2σ).

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.96.221302
DOI:
10.1103/PhysRevLett.96.221302
PACS:
98.80.Es, 11.30.Cp, 11.30.Er