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)

Detailed Description

Compute the fluxes \(F^i\) for the curved-space Irrotatational BNS equations on a spatial metric \(\gamma_{ij}\).

The documentation for this struct was generated from the following file:

Public Types