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In the electromagnetism of loop quantum gravity, two helicities of a photon have different phase velocities and group velocities, termed as ``vacuum birefringence''. Two novel phenomenons, ``peak doubling'' and ``depolarization'', are expected to appear for a linearly polarized light from astrophysical sources. We show that the criteria to observe these two phenomenons are the same. Further, from recently observed γ-ray polarization from Cygnus X-1, we obtain an upper limit ~8.7×10^-12 for the Lorentz-violating parameter χ, which is the most firm constraint from well-known systems. We also suggest analyzing the possible existence of ``peak doubling'' through Fermi-LAT gamma-ray bursts.
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Shao et al. (2011) studied this question.
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