activity
20202026
most citedCalibrating Core Overshooting Parameters With Two-dimensional Hydrodynamical Simulations

34 citations · 66 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2024★ 4 cited

Performance of high-order Godunov-type methods in simulations of astrophysical low Mach number flows

G. Leidi, R. Andrassy, W. Barsukow +3

High-order Godunov methods for gas dynamics have become a standard tool for simulating different classes of astrophysical flows. Their accuracy is mostly determined by the spatial…

astro-ph.SR2023★ 9 cited

Turbulent dynamo action and its effects on the mixing at the convective boundary of an idealized oxygen-burning shell

G. Leidi, R. Andrassy, J. Higl +2

Convection is one of the most important mixing processes in stellar interiors. Hydrodynamic mass entrainment can bring fresh fuel from neighboring stable layers into a convection z…

astro-ph.SR2023★ 2 cited

Towards a self-consistent model of the convective core boundary in upper main sequence stars. Part I: 2.5D and 3D simulations

R. Andrassy, G. Leidi, J. Higl +3

There is strong observational evidence that the convective cores of intermediate-mass and massive main sequence stars are substantially larger than those predicted by standard stel…

astro-ph.SR2022★ 17 cited

A finite-volume scheme for modeling compressible magnetohydrodynamic flows at low Mach numbers in stellar interiors

G. Leidi, C. Birke, R. Andrassy +5

Fully compressible magnetohydrodynamic (MHD) simulations are a fundamental tool for investigating the role of dynamo amplification in the generation of magnetic fields in deep conv…

astro-ph.SR2021

Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes

R. Andrassy, J. Higl, H. Mao +18

Our ability to predict the structure and evolution of stars is in part limited by complex, 3D hydrodynamic processes such as convective boundary mixing. Hydrodynamic simulations he…

astro-ph.SR2021

Well-balanced treatment of gravity in astrophysical fluid dynamics simulations at low Mach numbers

P. V. F. Edelmann, L. Horst, J. P. Berberich +5

Accurate simulations of flows in stellar interiors are crucial to improving our understanding of stellar structure and evolution. Because the typically slow flows are merely tiny p…