SpECTRE  v2026.04.01
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BnsInitialData::Fluxes Struct Reference

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
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 \(\gamma_{ij}\).

See also
IrrotationalBns::FirstOrderSystem

Member Typedef Documentation

◆ argument_tags

using BnsInitialData::Fluxes::argument_tags
Initial value:
tmpl::list<gr::Tags::InverseSpatialMetric<DataVector, 3>,
The stress-energy corresponding to the rotation shift.
Definition Tags.hpp:36

The documentation for this struct was generated from the following file:
  • src/Elliptic/Systems/BnsInitialData/Equations.hpp