248 citations · 2.3k across the 78 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…
Chemical complexity in astrophysical simulations: optimization and reduction techniques
T. Grassi, S. Bovino, D. Schleicher +1
Chemistry has a key role in the evolution of the interstellar medium (ISM), so it is highly desirable to follow its evolution in numerical simulations. However, it may easily domin…
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…
LiHe in the early Universe: a full assessment of its reaction network and final abundances
Stefano Bovino, Roman Curik, Daniele Galli +2
We present the results of quantum calculations based on entirely ab initio methods for a variety of molecular processes and chemical reactions involving the LiHe ionic polar mo…
Complexity reduction of astrochemical networks
T. Grassi, S. Bovino, F. A. Gianturco +2
We present a new computational scheme aimed at reducing the complexity of the chemical networks in astrophysical models, one which is shown to markedly improve their computational…