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000874408 041__ $$aEnglish
000874408 1001_ $$0P:(DE-HGF)0$$aWittor, Denis$$b0$$eCorresponding author
000874408 1112_ $$aNIC Symposium 2020$$cJülich$$d2020-02-27 - 2020-02-28$$wGermany
000874408 245__ $$aA Song of Shocks and Dynamo: Numerical Studies of a Galaxy Cluster Merger in the HIMAG Project
000874408 260__ $$aJülich$$bForschungszentrum Jülich GmbH Zentralbibliothek, Verlag$$c2020
000874408 29510 $$aNIC Symposium 2020
000874408 300__ $$a123 - 132
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000874408 4900_ $$aPublication Series of the John von Neumann Institute for Computing (NIC) NIC Series$$v50
000874408 520__ $$aWith ENZO simulations run on the Jülich supercomputers, we have investigated the evolution of magnetic fields in the largest cosmic structures (namely galaxy clusters and filaments connecting them) with unprecedented dynamical range. These simulations revealed the full development of the small-scale dynamo in Eulerian cosmological magneto-hydrodynamical simulations. The turbulent motions developed during the formation of clusters are energetic enough to foster the growth of magnetic fields by several orders of magnitude, starting from weak magnetic fields up to strengths of ~ $\mu$G as observed. Furthermore, shock waves are launched during cluster formation and they are able to accelerate cosmic-ray electrons, that emit in the radio wavelengths. Radio observations of this emission provide information on the local magnetic field strength. We have incorporated, for the first time, the cooling of cosmic-ray electrons when modelling this emission. In this contribution, we present our advances in modelling these physical processes. Here, we mostly focus on the most interesting object in our sample of galaxy clusters, which shows the complexity of magnetic fields and the potential of existing and future multi-wavelengths observations in the study of the weakly collisional plasma on ~ Megaparsecs scales.
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000874408 7001_ $$0P:(DE-HGF)0$$aDomínguez-Fernández, Paola$$b1
000874408 7001_ $$0P:(DE-HGF)0$$aVazza, Franco$$b2
000874408 7001_ $$0P:(DE-HGF)0$$aBrüggen, Marcus$$b3
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000874408 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$aUniveritá de Bologna$$b0
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000874408 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$aHamburger Sternwarte$$b1
000874408 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$aUniversitá di Bologna$$b2
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000874408 9201_ $$0I:(DE-Juel1)NIC-20090406$$kNIC$$lJohn von Neumann - Institut für Computing$$x0
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