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Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
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Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
classification
astro-ph.GA
astro-ph.HE
keywords
cosmicraysgalaxieslarge-scalemodelingstarburstultrahigh-energyaccelerated
read the original abstract
The Pierre Auger Collaboration has provided a compelling indication for a possible correlation between the arrival directions of ultrahigh-energy cosmic rays and nearby starburst galaxies. Herein we show how the latest large-scale modeling of starburst galaxies is compatible with the cosmic rays producing the anisotropy signal being accelerated at the terminal shock of superwinds.
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