SpECTRE
v2025.03.17
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Compute the time derivative of the conserved variables for the Newtonian Euler system. More...
#include <TimeDerivativeTerms.hpp>
Public Types | |
using | temporary_tags = implementation defined |
using | argument_tags = implementation defined |
Static Public Member Functions | |
static evolution::dg::TimeDerivativeDecisions< Dim > | apply (const gsl::not_null< Scalar< DataVector > * > non_flux_terms_dt_mass_density, const gsl::not_null< tnsr::I< DataVector, Dim > * > non_flux_terms_dt_momentum_density, const gsl::not_null< Scalar< DataVector > * > non_flux_terms_dt_energy_density, const gsl::not_null< tnsr::I< DataVector, Dim > * > mass_density_cons_flux, const gsl::not_null< tnsr::IJ< DataVector, Dim > * > momentum_density_flux, const gsl::not_null< tnsr::I< DataVector, Dim > * > energy_density_flux, const gsl::not_null< Scalar< DataVector > * > enthalpy_density, const Scalar< DataVector > &mass_density_cons, const tnsr::I< DataVector, Dim > &momentum_density, const Scalar< DataVector > &energy_density, const tnsr::I< DataVector, Dim > &velocity, const Scalar< DataVector > &pressure, const Scalar< DataVector > &specific_internal_energy, const EquationsOfState::EquationOfState< false, 2 > &eos, const tnsr::I< DataVector, Dim > &coords, const double time, const Sources::Source< Dim > &source) |
Compute the time derivative of the conserved variables for the Newtonian Euler system.