Computes the rest mass density $ρ$ , electron fraction $Y_{e}$ , temperature $T$ , Lorentz factor times the spatial velocity $W v^{i}$ , magnetic field $B^{i}$ , and the divergence cleaning field $Φ$ so they can be used for reconstruction. More...

#include <PrimitiveGhostData.hpp>

Public Types
using	return_tags = implementation defined

using	argument_tags = implementation defined

Static Public Member Functions
static DataVector	apply (const Variables< hydro::grmhd_tags< DataVector > > &prims, size_t rdmp_size)

Detailed Description

Computes the rest mass density $ρ$ , electron fraction $Y_{e}$ , temperature $T$ , Lorentz factor times the spatial velocity $W v^{i}$ , magnetic field $B^{i}$ , and the divergence cleaning field $Φ$ so they can be used for reconstruction.

The computation copies the data from the primitive variables to a new Variables and computes $W v^{i}$ . In the future we will likely want to elide this copy but that requires support from the actions.

This mutator is passed to evolution::dg::subcell::Actions::SendDataForReconstruction.

The documentation for this class was generated from the following file:

src/Evolution/Systems/GrMhd/ValenciaDivClean/Subcell/PrimitiveGhostData.hpp

Public Types

Static Public Member Functions

Detailed Description