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Kinetic Simulations of Cosmic-Ray-modified Shocks. II. Particle Spectra
Journal article   Peer reviewed

Kinetic Simulations of Cosmic-Ray-modified Shocks. II. Particle Spectra

Damiano Caprioli, Colby C. Haggerty and Pasquale Blasi
The Astrophysical journal, Vol.905(1), p.2
12/01/2020
DOI: 10.3847/1538-4357/abbe05
url
https://doi.org/10.3847/1538-4357/abbe05View
Published (Version of record) Open Access

Abstract

Diffusive shock acceleration is a prominent mechanism for producing energetic particles in space and in astrophysical systems. Such energetic particles have long been predicted to affect the hydrodynamic structure of the shock, in turn leading to CR spectra flatter than the test-particle prediction. However, in this work along with a companion paper, we use self-consistent hybrid (kinetic ion-fluid electron) simulations to show for the first time how CR-modified shocks actually produce steeper spectra. The steepening is driven by the enhanced advection of CRs embedded in magnetic turbulence downstream of the shock, in what we call the "postcursor." These results are consistent with multiwavelength observations of supernovae and supernova remnants and have significant phenomenological implications for space/astrophysical shocks in general.
Cosmic rays Galactic cosmic rays Plasma astrophysics Plasma physics Shocks Supernova remnants Supernovae

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