249 citations · 1.7k across the 41 of their papers we have counts for
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The Small-Scale Dynamo at Low Magnetic Prandtl Numbers
Jennifer Schober, Dominik Schleicher, Stefano Bovino +1
The present-day Universe is highly magnetized, even though the first magnetic seed fields were most probably extremely weak. To explain the growth of the magnetic field strength ov…
Turbulent magnetic field amplification from the smallest to the largest magnetic Prandtl numbers
Stefano Bovino, Dominik R. G. Schleicher, Jennifer Schober
The small-scale dynamo provides a highly efficient mechanism for the conversion of turbulent into magnetic energy. In astrophysical environments, such turbulence often occurs at hi…
Magnetic fields during high redshift structure formation
Dominik R. G. Schleicher, Muhammad Latif, Jennifer Schober +6
We explore the amplification of magnetic fields in the high-redshift Universe. For this purpose, we perform high-resolution cosmological simulations following the formation of prim…
Small-Scale Dynamo Action in Primordial Halos
Jennifer Schober, Dominik R. G. Schleicher, Ralf S. Klessen +4
The first galaxies form due to gravitational collapse of primordial halos. During this collapse, weak magnetic seed fields get amplified exponentially by the small-scale dynamo - a…
The Small-Scale Dynamo and Non-Ideal MHD in Primordial Star Formation
Jennifer Schober, Dominik Schleicher, Christoph Federrath +3
We study the amplification of magnetic fields during the formation of primordial halos. The turbulence generated by gravitational infall motions during the formation of the first s…