Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(488), p. 2466-2472, 2019
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Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
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Abstract
Abstract We show that the energy required to turbulently amplify magnetic field during cosmic ray (CR) acceleration by shocks extracts energy from the CR and steepens the CR energy spectrum.
