Numerical modeling of time-dependent cosmic-ray advection and diffusion in spherically symmetric wind bubbles shows escaping spectra harder than E^{-2} during the wind-driven phase, with low-energy suppression depending on the turbulence model.
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astro-ph.HE 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
SKA-Low augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.
SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.
citing papers explorer
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Time-dependent cosmic-ray escape from wind bubbles: hard spectra formation
Numerical modeling of time-dependent cosmic-ray advection and diffusion in spherically symmetric wind bubbles shows escaping spectra harder than E^{-2} during the wind-driven phase, with low-energy suppression depending on the turbulence model.
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Origins of Cosmic Rays in the Galactic-extragalactic Transition Energy Range
SKA-Low augmented with particle detectors is well suited to measure cosmic ray mass composition in the Galactic-extragalactic transition energy range, building on LOFAR experience.
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Understanding Pulsar Wind Nebulae with the SKA
SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.