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| SpecInitialData (const SpecInitialData &rhs) |
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SpecInitialData & | operator= (const SpecInitialData &rhs) |
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| SpecInitialData (SpecInitialData &&)=default |
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SpecInitialData & | operator= (SpecInitialData &&)=default |
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| SpecInitialData (std::string data_directory, std::unique_ptr< equation_of_state_type > equation_of_state, double density_cutoff, double atmosphere_density, std::optional< double > electron_fraction) |
| auto | get_clone () const -> std::unique_ptr< evolution::initial_data::InitialData > override |
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const equation_of_state_type & | equation_of_state () const |
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template<typename DataType, typename... Tags> |
| tuples::TaggedTuple< Tags... > | variables (const tnsr::I< DataType, 3 > &x, tmpl::list< Tags... >) const |
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void | pup (PUP::er &) override |
template<size_t ThermodynamicDim>
class grmhd::AnalyticData::SpecInitialData< ThermodynamicDim >
Hydro initial data generated by SpEC.
This class loads numerical data written out by the SpEC initial data solver. It uses the spec::Exporter linked in from SpEC to interpolate to arbitrary grid points. The coordinates are assumed to be in SpEC's "grid" frame. We interpolate the following quantities:
- "g": spatial metric
- "K": (lower) extrinsic curvature
- "Lapse": lapse
- "Shift": (upper) shift
- "BaryonDensity": rest mass density
- "u_i": lower spatial four-velocity
The remaining hydro quantities are computed from the interpolated data and the equation of state. The magnetic field is set to zero and the electron fraction is set to a constant read from the input file.