Published September 1999 | Version v1
Journal article

Limits to Quantum Gravity Effects on Energy Dependence of the Speed of Light from Observations of TeV Flares in Active Galaxies

  • 1. Oxford University, Oxford (United Kingdom)
  • 2. University College, Dublin (Ireland)
  • 3. Washington University, St. Louis, Missouri 63130 (United States)
  • 4. Iowa State University, Ames, Iowa 50011 (United States)
  • 5. Maynooth University, Maynooth (Ireland)
  • 6. Purdue University, West Lafayette, Indiana 47907 (United States)
  • 7. University of Leeds, Leeds (United Kingdom)
  • 8. California Institute of Technology, California 91125 (United States)
  • 9. University of Utah, Salt Lake City, Utah 84112 (United States)
  • 10. Galway-Mayo Institute of Technology, Galway (Ireland)
  • 11. Whipple Observatory, Amado, Arizona 85645 (United States)

Description

We have used data from a TeV γ -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 1016 GeV. The limits derived here indicate this energy scale to be in excess of 6x1016 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. copyright 1999 The American Physical Society

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
83
Journal Issue
11
Journal Page Range
p. 2108-2111
ISSN
0031-9007
CODEN
PRLTAO