A dust-driven streaming instability downstream of supernova remnant shocks can amplify magnetic fields enough to explain observed X-ray filaments, potentially eliminating the need for upstream field amplification and associated ultra-high-energy cosmic-ray acceleration.
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Dust-driven streaming instability and magnetic field amplification downstream of supernova remnant shocks
A dust-driven streaming instability downstream of supernova remnant shocks can amplify magnetic fields enough to explain observed X-ray filaments, potentially eliminating the need for upstream field amplification and associated ultra-high-energy cosmic-ray acceleration.