Add the sources \(S_A\) for the curved-space Irrotatioanl BNS equation on a spatial metric \(\gamma_{ij}\). More...

#include <Equations.hpp>

Public Types
using	argument_tags = tmpl::list< Tags::DerivLogLapseTimesDensityOverSpecificEnthalpy< DataVector >, gr::Tags::SpatialChristoffelSecondKindContracted< DataVector, 3 > >

Static Public Member Functions
static void	apply (gsl::not_null< Scalar< DataVector > * > equation_for_potential, const tnsr::i< DataVector, 3 > &log_deriv_lapse_times_density_over_specific_enthalpy, const tnsr::i< DataVector, 3 > &christoffel_contracted, const Scalar< DataVector > &velocity_potential, const tnsr::I< DataVector, 3 > &flux_for_potential)

Detailed Description

Add the sources \(S_A\) for the curved-space Irrotatioanl BNS equation on a spatial metric \(\gamma_{ij}\).

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

Public Types