301 citations · 6.3k across the 162 of their papers we have counts for
165 papers
Global 3D simulations of convection and dynamos in Red Giants
Carolina Ortiz-Rodríguez, Petri Käpylä, Juan Pablo Hidalgo +2
Understanding the internal dynamics of red giants is essential for studying angular momentum transport and magnetic field generation during stellar evolution. We present three-dime…
Magnetic fields in extreme primordial halos: turbulent collapse and implications for early quasar formation
V. B. Díaz, D. R. G. Schleicher, M. A. Latif +1
It is sometimes suggested that the most massive quasars at high redshift may have formed from rare high-sigma peaks in the cosmic density field. We explore here the evolution in a…
Magnetic field amplification in massive primordial halos: Influence of Lyman-Werner radiation
V. B. Díaz, D. R. G. Schleicher, M. A. Latif +2
The potential importance of magnetic fields during structure formation and gravitational collapse in the early Universe has been shown in several studies. In particular, magnetic f…
Magnetic braking during direct collapse black hole formation
Muhammad A. Latif, Dominik R. G. Schleicher
Magnetic fields are expected to be efficiently amplified during the formation of the first massive black holes via the small-scale dynamo and in the presence of strong accretion sh…
Survival of fossil fields during the pre-main sequence evolution of intermediate-mass stars
Dominik R. G. Schleicher, Juan Pablo Hidalgo, Daniele Galli
Chemically peculiar Ap and Bp stars host strong large-scale magnetic fields in the range of ~G up to ~kG, which are often considered to be the origin of fossil magnetic fi…
Effects of the centrifugal force in stellar dynamo simulations
Felipe H. Navarrete, Petri J. Käpylä, Dominik R. G. Schleicher +1
The centrifugal force is often omitted from simulations of stellar convection either for numerical reasons or because it is assumed to be weak compared to the gravitational force.…