SpECTRE
v2024.08.03
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Compute the fluxes \(F^i\) for the curved-space Irrotatational BNS equations on a spatial metric \(\gamma_{ij}\). More...
#include <Equations.hpp>
Public Types | |
using | argument_tags = tmpl::list< gr::Tags::InverseSpatialMetric< DataVector, 3 >, Tags::RotationalShiftStress< DataVector > > |
using | volume_tags = tmpl::list<> |
using | const_global_cache_tags = tmpl::list<> |
Static Public Member Functions | |
static void | apply (gsl::not_null< tnsr::I< DataVector, 3 > * > flux_for_potential, const tnsr::II< DataVector, 3 > &inverse_spatial_metric, const tnsr::II< DataVector, 3 > &rotational_shift_stress, const Scalar< DataVector > &velocity_potential, const tnsr::i< DataVector, 3 > &velocity_potential_gradient) |
static void | apply (gsl::not_null< tnsr::I< DataVector, 3 > * > flux_on_face, const tnsr::II< DataVector, 3 > &inverse_spatial_metric, const tnsr::II< DataVector, 3 > &rotational_shift_stress, const tnsr::i< DataVector, 3 > &face_normal, const tnsr::I< DataVector, 3 > &face_normal_vector, const Scalar< DataVector > &velocity_potential) |
Compute the fluxes \(F^i\) for the curved-space Irrotatational BNS equations on a spatial metric \(\gamma_{ij}\).