The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
Galactic synchrotron emissions above 20 MHz can set tighter upper limits on the abundance of primordial black holes with masses above 10^16 grams than previous cosmic-ray electron data.
citing papers explorer
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Geometry, Not Calorimetry, Drives the Radio/Infrared/Gamma-Ray Correlation
The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
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Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection
Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
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Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions
Galactic synchrotron emissions above 20 MHz can set tighter upper limits on the abundance of primordial black holes with masses above 10^16 grams than previous cosmic-ray electron data.