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A C++ low Mach number stellar hydrodynamics code

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If a problem is restarted from a checkpoint output at the 0th timestep, then the timestep evolution itself appears to run fine, however the time at the end of the...

This implements an additional -\overline{\lambda}\rho **g** term in the momentum equation that should lead to better energy conservation when hydrostatic equilibrium is enforced (the form of the term(s) may be...

This adds the option to use a thermodynamically consistent temperature by setting `use_correct_temp = true`. Two options have also been added to include the corrected tfrom[p|h] in the plotfile. At...

This issue serves to track Microphysics starkiller-astro/Microphysics#496 as it applies to MAESTROeX. For Strang integration, we will switch from integrating (T, X_k) to integrating (e, X_k) in the reaction networks....

Compile `science/ecsn` as: ``` make COMP=gnu USE_OMP=FALSE ``` then run a single-level test as: ``` mpiexec -n 16 ./Maestro3d.gnu.MPI.ex input_ecsn amr.max_level=0 ``` Looking at plotfile 0, fextrema shows: ``` Hnuc...

We need to OpenMP the routines in MaestroRegrid.cpp. It used to be implemented but would crash the planar multilevel with MPI+OpenMP.

Routines offloaded to the GPU now take the 1d base state mapped to a 3d MultiFab. This mapping is often done within the C++ wrapper function of these routines, which...

GPU

This would require using the AMReX tensor solve since div(u) != 0.

Hello, Im looking to develop some capability to model the dynamics of hot bubble motion in a stratified atmosphere, where the scale height is an important consideration, and the densities/temperatures...

question :grey_question:

The docs have not been updated much to reflect the changes in MAESTROeX vs MAESTRO, so there are a few sections where they should be updated

documentation :book: