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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格式: | Journal article |
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American Physical Society
2017
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