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CERN Experiment Recreates Blazar Pair Cascades, Points to Intergalactic Magnetic Fields

The results favor weak intergalactic magnetic fields as the reason Fermi has not seen the expected GeV gamma rays.

Overview

  • An Oxford-led team used CERN’s Super Proton Synchrotron at the HiRadMat facility to generate electron–positron pairs and drive them through a meter-long ambient plasma as a scaled analogue of blazar cascades.
  • Measurements showed the pair beam stayed narrow with minimal self-generated magnetic fields, indicating suppressed beam–plasma instabilities in the laboratory setup.
  • The findings imply such instabilities are too weak to account for the missing secondary GeV emission from blazars, shifting weight toward deflection by weak intergalactic magnetic fields.
  • The study was published in the Proceedings of the National Academy of Sciences on November 3, 2025 (DOI: 10.1073/pnas.2513365122).
  • Researchers highlight unresolved questions about the origin of intergalactic magnetism and point to upcoming tests with facilities such as the Cherenkov Telescope Array Observatory.