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Simulating cosmic ray physics on a moving mesh

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We discuss new methods to integrate the cosmic ray (CR) evolution equations coupled to magnetohydrodynamics on an unstructured moving mesh, as realized in the massively parallel arepo code for cosmological simulations. We account for diffusive shock acceleration of CRs at resolved shocks and at supe...

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Main Authors: Pfrommer, Christoph (Author) , Pakmor, Rüdiger (Author) , Schaal, Kevin (Author) , Simpson, Christine M. (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2016, Volume: 465, Issue: 4, Pages: 4500-4529
ISSN:1365-2966
DOI:10.1093/mnras/stw2941
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2941
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Author Notes:C. Pfrommer, R. Pakmor, K. Schaal, C.M. Simpson and V. Springel
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Simulating cosmic ray physics on a moving mesh by Pfrommer, Christoph (Author) , Pakmor, Rüdiger (Author) , Schaal, Kevin (Author) , Springel, Volker (Author) ,


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