Limits to quantum gravity effects on energy dependence of the speed of light from observations of tev flares in active galaxies

S. D. Biller, A. C. Breslin, J. Buckley, M. Catanese, M. Carson, D. A. Carter-Lewis, M. F. Cawley, D. J. Fegan, J. Finley, J. A. Gaidos, A. M. Hillas, F. Krennrich, R. C. Lamb, R. Lessard, C. Masterson, J. E. Mc Enery, B. Mc Kernan, P. Moriarty, J. Quinn, H. J. RoseF. Samuelson, G. Sembroski, P. Skelton, T. C. Weekes

Research output: Contribution to a Journal (Peer & Non Peer)Articlepeer-review

234 Citations (Scopus)

Abstract

We have used data from a TeV gamma-ray flare associated with the active galaxy Markarian 421 to place bounds on the possible energy dependence of the speed of light in the context of an effective quantum gravitational energy scale. Recent theoretical work suggests that such an energy scale could be less than the Planck mass and perhaps as low as 10^16 GeV. The limits derived here indicate this energy scale to be in excess of 4×106 GeV for at least one approach to quantum gravity in the context of D-brane string theory. To the best of our knowledge this constitutes the first convincing limit on such phenomena in this energy regime.

Original languageEnglish
Pages (from-to)2108-2111
Number of pages4
JournalPhysical Review Letters
Volume83
Issue number11
DOIs
Publication statusPublished - 1 Jan 1999
Externally publishedYes

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