SpECTRE  v2025.03.17
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BnsInitialData::Fluxes Struct Reference

Compute the fluxes Fi for the curved-space Irrotatational BNS equations on a spatial metric γij. More...

#include <Equations.hpp>

Public Types

using argument_tags = implementation defined
 
using volume_tags = implementation defined
 
using const_global_cache_tags = implementation defined
 

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 Fi for the curved-space Irrotatational BNS equations on a spatial metric γij.

See also
IrrotationalBns::FirstOrderSystem

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