SpECTRE
v2024.05.11
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Compute the time derivative of the conserved variables for the Valencia formulation of the relativistic Euler equations. More...
#include <TimeDerivativeTerms.hpp>
Classes | |
struct | DensitizedStress |
struct | PressureLapseSqrtDetSpatialMetric |
struct | TildeSUp |
Static Public Member Functions | |
static void | apply (gsl::not_null< Scalar< DataVector > * >, gsl::not_null< Scalar< DataVector > * > non_flux_terms_dt_tilde_tau, gsl::not_null< tnsr::i< DataVector, Dim, Frame::Inertial > * > non_flux_terms_dt_tilde_s, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > tilde_d_flux, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > tilde_tau_flux, gsl::not_null< tnsr::Ij< DataVector, Dim, Frame::Inertial > * > tilde_s_flux, gsl::not_null< Scalar< DataVector > * > pressure_lapse_sqrt_det_spatial_metric, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > transport_velocity, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > tilde_s_up, gsl::not_null< tnsr::II< DataVector, Dim, Frame::Inertial > * > densitized_stress, gsl::not_null< Scalar< DataVector > * > temp_lapse, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > temp_shift, gsl::not_null< tnsr::ii< DataVector, Dim, Frame::Inertial > * > temp_spatial_metric, gsl::not_null< tnsr::II< DataVector, Dim, Frame::Inertial > * > temp_inv_spatial_metric, const Scalar< DataVector > &tilde_d, const Scalar< DataVector > &tilde_tau, const tnsr::i< DataVector, Dim, Frame::Inertial > &tilde_s, const Scalar< DataVector > &lapse, const tnsr::I< DataVector, Dim, Frame::Inertial > &shift, const Scalar< DataVector > &sqrt_det_spatial_metric, const Scalar< DataVector > &pressure, const tnsr::I< DataVector, Dim, Frame::Inertial > &spatial_velocity, const tnsr::i< DataVector, Dim, Frame::Inertial > &d_lapse, const tnsr::iJ< DataVector, Dim, Frame::Inertial > &d_shift, const tnsr::ijj< DataVector, Dim, Frame::Inertial > &d_spatial_metric, const tnsr::II< DataVector, Dim, Frame::Inertial > &inv_spatial_metric, const tnsr::ii< DataVector, Dim, Frame::Inertial > &extrinsic_curvature, const tnsr::ii< DataVector, Dim, Frame::Inertial > &spatial_metric) |
Compute the time derivative of the conserved variables for the Valencia formulation of the relativistic Euler equations.