New radio observations at cold fronts in galaxy clusters lead to the proposal that magnetic reconnection, rather than Fermi acceleration, re-accelerates particles at these contact discontinuities.
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2026 2representative citing papers
A research framework combining XRISM turbulent velocity maps with SKA rotation measure grids to break degeneracies between magnetic field strength and cosmic-ray energetics in galaxy clusters.
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Magnetic Reconnection in Galaxy Clusters
New radio observations at cold fronts in galaxy clusters lead to the proposal that magnetic reconnection, rather than Fermi acceleration, re-accelerates particles at these contact discontinuities.
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Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM
A research framework combining XRISM turbulent velocity maps with SKA rotation measure grids to break degeneracies between magnetic field strength and cosmic-ray energetics in galaxy clusters.