Simulations show that primordial magnetic fields with different coherence scales produce unique angular autocorrelation signatures in intergalactic rotation measures, ranging from 90-degree correlations for large-scale models to sharp drops at 0.1-degree scales for small-scale stochastic models.
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Magnetized cosmic web filaments suppress UHECR proton flux below 3×10^19 eV, producing magnetic horizon radii of ~50 Mpc at 10^18 eV and ~150 Mpc at 10^19 eV.
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Simulated Rotation Measure Sky from Primordial Magnetic Fields
Simulations show that primordial magnetic fields with different coherence scales produce unique angular autocorrelation signatures in intergalactic rotation measures, ranging from 90-degree correlations for large-scale models to sharp drops at 0.1-degree scales for small-scale stochastic models.
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The Impact of the Magnetised Cosmic Web on Ultra High Energy Cosmic Ray Propagation
Magnetized cosmic web filaments suppress UHECR proton flux below 3×10^19 eV, producing magnetic horizon radii of ~50 Mpc at 10^18 eV and ~150 Mpc at 10^19 eV.