Implications of strong intergalactic magnetic fields for ultrahigh-energy cosmic-ray astronomy

We study the propagation of ultra-high-energy cosmic rays in the magnetised cosmic web. We focus on the particular case of highly magnetised voids ($B \sim \text{nG}$), using the upper bounds from the Planck satellite. The cosmic web was obtained from purely magnetohydrodynamical cosmological simula...

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Detalhes bibliográficos
Principais autores: Batista, R, Shin, M, Devriendt, J, Semikoz, D, Sigl, G
Formato: Journal article
Publicado em: American Physical Society 2017