The study of low Mach number limits in fluid dynamics, particularly in the context of the Navier-Stokes equations and magnetohydrodynamics (MHD), is crucial for understanding the behavior of ...
"In 5,000 years, the mass of the most massive star is 65 solar masses in the RMHD radiation magnetohydrodynamics simulation, compared to 120 solar masses in simulations without magnetic fields ...
Optimization of Gas Flows Ensures Effective Heat Transport “At first glance, this project has less to do with the fluid mechanics that we usually deal with at the institute,” explains HZDR engineer Dr ...
My research is primarily focused on the development of advanced numerical methods to model core-collapse supernovae — in particular neutrino radiation hydrodynamics and magnetohydrodynamics. These ...
The Computational Mechanics and Geometry Laboratory (CMGLab), led by Dr. John A. Evans of the Ann and H.J. Smead Department of Aerospace Engineering Sciences, pioneers new approaches to the modeling, ...
There has never been a more exciting time to study the exciting discipline of physics, spanning the workings of the sub-atomic world to the ever-expanding universe. The BS Physics Program in the ...
In the forefront of quantitative solar physics research using large-aperture ground-based solar optical telescopes, high-contrast observation along with high-accuracy polarimetric measurement in the ...
Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.
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