Presents 24 AREPO+IllustrisTNG zoom-in simulations of clusters above 10^15 solar masses showing converged magnetic fields with volume-averaged plasma beta approximately 100 inside R200 after z~1.2, declining Faraday rotation profiles, and intermittent Braginskii heating approaching cooling rates in
2020 b , , 899, 115, 10.3847/1538-4357/aba7ba
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Direct numerical simulations find no vorticity generation attributable to the collapse flow itself when starting from irrotational turbulence in a barotropic, non-magnetized fluid.
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The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating
Presents 24 AREPO+IllustrisTNG zoom-in simulations of clusters above 10^15 solar masses showing converged magnetic fields with volume-averaged plasma beta approximately 100 inside R200 after z~1.2, declining Faraday rotation profiles, and intermittent Braginskii heating approaching cooling rates in
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No evidence of vorticity production from initially irrotational turbulent gravitational collapse
Direct numerical simulations find no vorticity generation attributable to the collapse flow itself when starting from irrotational turbulence in a barotropic, non-magnetized fluid.