Compute the time derivative of the conserved variables for the Valencia formulation of the GRMHD equations with divergence cleaning. More...
#include <TimeDerivativeTerms.hpp>
Classes | |
| struct | DensitizedStress |
| struct | EnthalpyTimesDensityWSquaredPlusBSquared |
| struct | LapseTimesbOverW |
| struct | MagneticFieldOneForm |
| struct | OneOverLorentzFactorSquared |
| struct | PressureStar |
| struct | PressureStarLapseSqrtDetSpatialMetric |
| struct | TildeSUp |
Public Types | |
| using | temporary_tags = implementation defined |
| using | argument_tags = implementation defined |
Static Public Member Functions | |
| static evolution::dg::TimeDerivativeDecisions< 3 > | apply (gsl::not_null< Scalar< DataVector > * >, gsl::not_null< Scalar< DataVector > * >, gsl::not_null< Scalar< DataVector > * > non_flux_terms_dt_tilde_tau, gsl::not_null< tnsr::i< DataVector, 3, Frame::Inertial > * > non_flux_terms_dt_tilde_s, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > non_flux_terms_dt_tilde_b, gsl::not_null< Scalar< DataVector > * > non_flux_terms_dt_tilde_phi, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > tilde_d_flux, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > tilde_ye_flux, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > tilde_tau_flux, gsl::not_null< tnsr::Ij< DataVector, 3, Frame::Inertial > * > tilde_s_flux, gsl::not_null< tnsr::IJ< DataVector, 3, Frame::Inertial > * > tilde_b_flux, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > tilde_phi_flux, gsl::not_null< tnsr::i< DataVector, 3, Frame::Inertial > * > spatial_velocity_one_form, gsl::not_null< tnsr::i< DataVector, 3, Frame::Inertial > * > magnetic_field_one_form, gsl::not_null< Scalar< DataVector > * > magnetic_field_dot_spatial_velocity, gsl::not_null< Scalar< DataVector > * > magnetic_field_squared, gsl::not_null< Scalar< DataVector > * > one_over_w_squared, gsl::not_null< Scalar< DataVector > * > pressure_star, gsl::not_null< Scalar< DataVector > * > pressure_star_lapse_sqrt_det_spatial_metric, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > transport_velocity, gsl::not_null< tnsr::i< DataVector, 3, Frame::Inertial > * > lapse_b_over_w, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > tilde_s_up, gsl::not_null< tnsr::II< DataVector, 3, Frame::Inertial > * > densitized_stress, gsl::not_null< tnsr::ijj< DataVector, 3, Frame::Inertial > * > spatial_christoffel_first_kind, gsl::not_null< tnsr::Ijj< DataVector, 3, Frame::Inertial > * > spatial_christoffel_second_kind, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > trace_spatial_christoffel_second, gsl::not_null< Scalar< DataVector > * > h_rho_w_squared_plus_b_squared, gsl::not_null< Scalar< DataVector > * > temp_lapse, gsl::not_null< tnsr::I< DataVector, 3, Frame::Inertial > * > temp_shift, gsl::not_null< tnsr::II< DataVector, 3, Frame::Inertial > * > temp_inverse_spatial_metric, const Scalar< DataVector > &tilde_d, const Scalar< DataVector > &tilde_ye, const Scalar< DataVector > &tilde_tau, const tnsr::i< DataVector, 3, Frame::Inertial > &tilde_s, const tnsr::I< DataVector, 3, Frame::Inertial > &tilde_b, const Scalar< DataVector > &tilde_phi, const Scalar< DataVector > &lapse, const tnsr::I< DataVector, 3, Frame::Inertial > &shift, const Scalar< DataVector > &sqrt_det_spatial_metric, const tnsr::ii< DataVector, 3, Frame::Inertial > &spatial_metric, const tnsr::II< DataVector, 3, Frame::Inertial > &inv_spatial_metric, const tnsr::i< DataVector, 3, Frame::Inertial > &d_lapse, const tnsr::iJ< DataVector, 3, Frame::Inertial > &d_shift, const tnsr::ijj< DataVector, 3, Frame::Inertial > &d_spatial_metric, const Scalar< DataVector > &pressure, const tnsr::I< DataVector, 3, Frame::Inertial > &spatial_velocity, const Scalar< DataVector > &lorentz_factor, const tnsr::I< DataVector, 3, Frame::Inertial > &magnetic_field, const Scalar< DataVector > &rest_mass_density, const Scalar< DataVector > &electron_fraction, const Scalar< DataVector > &specific_internal_energy, const tnsr::ii< DataVector, 3, Frame::Inertial > &extrinsic_curvature, double constraint_damping_parameter) |
Compute the time derivative of the conserved variables for the Valencia formulation of the GRMHD equations with divergence cleaning.