If the photon dispersion relation is (pc)(2) = E-2 + E-3/E-QG, as suggested
in certain approaches to quantizing gravity, then high energy photons may
be unable to pair-create on cosmic microwave background (CBR) and infrared
background (IR) photons. If E-QG similar to 10(16) GeV, powerful sources of
TeV radiation, e.g. in AGNs, could be detectable out to large redshifts. (
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