Probing the IGMF with the Next Generation of Cherenkov Telescopes
Intergalactic space is believed to contain nonzero magnetic fields (the Intergalactic Magnetic Field: IGMF), which at scales of megaparsecs would have intensities below 10-9 G. Very high energy (VHE > 100 GeV) gamma-rays coming from blazars can produce e+e- pairs when interacting with the ext...
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| Autores principales: | Alonso, M.F., Supanitsky, A.D., Rovero, A.C. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v869_n1_p_Alonso |
| Aporte de: |
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