Issue |
A&A
Volume 483, Number 3, June I 2008
|
|
---|---|---|
Page(s) | 715 - 718 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361:200809410 | |
Published online | 19 March 2008 |
Testing CPT symmetry with CMB measurements
1
Institute of High Energy Physics, Chinese Academy of Science, PO Box 918-4, Beijing 100049, PR China e-mail: xiajq@mail.ihep.ac.cn
2
Department of Astronomy, School of Physics, Peking University, Beijing 100871, PR China
3
Fakultät für Physik, Universität Bielefeld, 33615 Bielefeld, Germany
Received:
17
January
2008
Accepted:
27
February
2008
Aims. We study the possibility of testing Charge-Parity-Time Reversal symmetry (CPT) with cosmic microwave background (CMB) measurements.
Methods. Working with an effective
lagrangian of the photon with CPT violation , which causes the polarization
vectors of the propagating CMB photons to be rotated, we determine
the rotation angle
using the BOOMERanG 2003 and the
WMAP3 angular power spectra.
Results. In this analysis, we have included
the newly-released TC and GC () information of WMAP3 and
found
deg at a
confidence level.
Conclusions. This result slightly increases the significance for the CPT
violation obtained in our previous paper (Feng et al. 2006)
deg (1σ). Furthermore, we
examine the constraint on the rotation angle from the simulated
polarization data with Planck precision. Our results show that the
future Planck measurement will be sensitive to
at
the level of 0.057 deg and will be able to test the CPT symmetry
with a higher precision.
Key words: cosmology: theory / cosmology: cosmic microwave background / cosmology: cosmological parameters
© ESO, 2008
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