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Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations

By H. E. S. S. and others
Magnetic fields in galaxies and galaxy clusters are believed to be the result of the amplification of intergalactic seed fields during the formation of large-scale structures in the universe. However, the origin, strength, and morphology of this intergalactic magnetic field (IGMF) remain unknown. Lower limits on (or indirect detection of)... Show more
June 8, 2023
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Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations
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