Injecting 10% of supernova energy as cosmic rays in a Parker-unstable galactic disk drives a longer-lived outflow and lowers the cosmic-ray calorimetric fraction when the magnetic field is well resolved.
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Cosmic-Ray Feedback from Supernovae in a Parker-Unstable Medium
Injecting 10% of supernova energy as cosmic rays in a Parker-unstable galactic disk drives a longer-lived outflow and lowers the cosmic-ray calorimetric fraction when the magnetic field is well resolved.