Simulating cosmic ray physics on a moving mesh
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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| Hauptverfasser: | , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 465, Heft: 4, Pages: 4500-4529 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw2941 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw2941
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| Verfasserangaben: | C. Pfrommer, R. Pakmor, K. Schaal, C.M. Simpson and V. Springel |
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