The key step was to adapt a 'covariant' regularization that looks like
where the time derivative on the RHS is new compared to previous attempts. We approximate
Note that this is not truely covariant, but
This PR adds example parameter files that allow to reproduce the SRHD tests from https://arxiv.org/pdf/2202.08839.pdf. To run the blastwave2
test it was important to add correct the evolved variable tau
whenever the energy density eps
turned slightly negative, as suggested in https://arxiv.org/pdf/2005.01821.pdf III.A.
What is interesting is that atm we don't need an atmosphere description, but that's probably because those tests do not examine low densities.
Side note: Realized that !75 (merged) promoted Mesh
to a parameteric type and now most of the HRSC and TCI structs suffer from type instabilities. Need to fix this in a separate PR.