The time step constraint in radiation hydrodynamics

DOI10.1080/03091929.2019.1676894zbMath1482.76151OpenAlexW2912258785WikidataQ114640039 ScholiaQ114640039MaRDI QIDQ5065700

Upasana Das, Axel Brandenburg

Publication date: 22 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091929.2019.1676894

zbMATH Keywords

convectionnumerical stabilityradiative coolingaccretion discshot stars

Mathematics Subject Classification ID

Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

Introduction

Uses Software

• ZEUS
• CO5BOLD
• Athena
• HERACLES
• DISPATCH

Cites Work

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• Radiative transfer in decomposed domains
• A 3D MHD model of astrophysical flows: Algorithms, tests and parallelisation
• Intermittent heating in the solar corona employing a 3D MHD model
• Effects of a subadiabatic layer on convection and dynamos in spherical wedge simulations
• Sensitivity to luminosity, centrifugal force, and boundary conditions in spherical shell convection
• A Method for the Numerical Calculation of Hydrodynamic Shocks

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