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Castro (Compressible Astrophysics): An adaptive mesh, astrophysical compressible (radiation-, magneto-) hydrodynamics simulation code for massively parallel CPU and GPU architectures.

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Currently, in the ppm tracing, we use the reference states in computing the eigenvectors. But this means that, since we include sources now in the reference states, that all the...

hydro

We should merge the 2 ppm tracing routines, as most of the code is redundant.

hydro
clean-up

Sometimes we only model a portion of a star, with the surface outside of the computational domain. We used to have the ability to spherically average the star on the...

hackathon

The _prob_params script (and perhaps later on _cpp_parameters and the extern variables) should be switched to a key = value format so that we can more easily add fields in...

hackathon

Right now, if the interface prediction for density is > `small_dens`, we set the interface state to density. But this will yield a thermodynamically inconsistent state. A better approach might...

We have 2 true SDC detonation tests in the test suite (one 2nd order and the other 4th order). Currently, they have VODE errors after 12 - 14 timestep. This...

For generating initial models at runtime, it would be useful to know already when we call `probinit` what the finest level `dx(:)` is. One way we could do this is...

## PR summary ## PR motivation ## PR checklist - [ ] test suite needs to be run on this PR - [ ] this PR will change answers in...

## PR summary This does a better(?) implementation of the CMA method. By working on the interface states directly, it will be in effect for the transverse flux differences and...

hydro

Right now we carry around 3 area MFs + 1 volume MF. These are not used very widely, and it seems that with the C++ conversion, we could create an...