Abstract
Cosmological simulations of galaxy formation provide the most powerful technique for calculating the non-linear evolution of cosmic structure formation. This approach starts from initial conditions determined during the Big Bang – which are precisely specified in the cosmological standard model – and evolves them forward in time to the present epoch, thereby providing detailed predictions that test the cosmological paradigm. Here we report first preliminary results from a new generation of hydrodynamical simulations that excel with new physics, enlarged dynamic range and more accurate numerical techniques. The simulations of our ongoing Illustris++ project on HazelHen successfully reproduce the appearance of a red sequence of galaxies that are quenched by accreting supermassive black holes, while at the same time yielding a population of disk galaxies with properties that closely match observational data. Also, we are able to predict the amplification of magnetic fields through small-scale dynamo processes in realistic simulations of large galaxy populations, thereby providing novel predictions for the field strength and topology expected for galaxies of different size and type.
References
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Acknowledgements
The authors gratefully acknowledge computer time through the project GCS-ILLU on Hornet/HazelHen at HLRS. We acknowledge financial support through subproject EXAMAG of the Priority Programme 1648 ‘SPPEXA’ of the German Science Foundation, and through the European Research Council through ERC-StG grant EXAGAL-308037, and we would like to thank the Klaus Tschira Foundation.
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Springel, V. et al. (2016). The Illustris++ Project: The Next Generation of Cosmological Hydrodynamical Simulations of Galaxy Formation. In: Nagel, W.E., Kröner, D.H., Resch, M.M. (eds) High Performance Computing in Science and Engineering ´16. Springer, Cham. https://doi.org/10.1007/978-3-319-47066-5_1
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DOI: https://doi.org/10.1007/978-3-319-47066-5_1
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