#include <StarSurface.hpp>

Public Types
using	options = tmpl::list<>

using	argument_tags = tmpl::list< gr::Tags::Lapse< DataVector >, BnsInitialData::Tags::RotationalShift< DataVector >, BnsInitialData::Tags::EulerEnthalpyConstant, domain::Tags::FaceNormal< 3 > >

using	volume_tags = tmpl::list< BnsInitialData::Tags::EulerEnthalpyConstant >

using	argument_tags_linearized = tmpl::list<>

using	volume_tags_linearized = tmpl::list<>

Public Member Functions
	StarSurface (const StarSurface &)=default

StarSurface &	operator= (const StarSurface &)=default

	StarSurface (StarSurface &&)=default

StarSurface &	operator= (StarSurface &&)=default

std::unique_ptr< domain::BoundaryConditions::BoundaryCondition >	get_clone () const override

	StarSurface (const Options::Context &context)

std::vector< elliptic::BoundaryConditionType >	boundary_condition_types () const override

void	pup (PUP::er &p) override

Public Member Functions inherited from elliptic::BoundaryConditions::BoundaryCondition< 3 >
	BoundaryCondition (const BoundaryCondition &)=default

	BoundaryCondition (BoundaryCondition &&)=default

BoundaryCondition &	operator= (const BoundaryCondition &)=default

BoundaryCondition &	operator= (BoundaryCondition &&)=default

virtual std::vector< elliptic::BoundaryConditionType >	boundary_condition_types () const=0

Public Member Functions inherited from domain::BoundaryConditions::BoundaryCondition
	BoundaryCondition (BoundaryCondition &&)=default

BoundaryCondition &	operator= (BoundaryCondition &&)=default

	BoundaryCondition (const BoundaryCondition &)=default

BoundaryCondition &	operator= (const BoundaryCondition &)=default

	BoundaryCondition (CkMigrateMessage *const msg)

	WRAPPED_PUPable_abstract (BoundaryCondition)

virtual auto	get_clone () const -> std::unique_ptr< BoundaryCondition >=0

Static Public Member Functions
static void	apply (gsl::not_null< Scalar< DataVector > * > velocity_potential, gsl::not_null< Scalar< DataVector > * > n_dot_flux_for_potential, const tnsr::i< DataVector, 3 > &deriv_velocity_potential, const Scalar< DataVector > &lapse, const tnsr::I< DataVector, 3 > &rotational_shift, double euler_enthalpy_constant, const tnsr::i< DataVector, 3 > &normal)

static void	apply_linearized (gsl::not_null< Scalar< DataVector > * > velocity_potential_correction, gsl::not_null< Scalar< DataVector > * > n_dot_flux_for_potential_correction, const tnsr::i< DataVector, 3 > &deriv_velocity_potential)

Static Public Attributes
static constexpr Options::String	help

Static Public Attributes inherited from elliptic::BoundaryConditions::BoundaryCondition< 3 >
static constexpr size_t	volume_dim

Detailed Description

Impose StarSurface boundary conditions:

\[ n_i F^i = \frac{C}{\alpha^2} B^i n_i. \]

The boundary condition results from requiring the conservation equations be regular at the surface of the neutron star. See [13] 15.79.

Member Function Documentation

std::vector< elliptic::BoundaryConditionType > BnsInitialData ::BoundaryConditions::StarSurface::boundary_condition_types ( ) const

inlineoverridevirtual

std::unique_ptr< domain::BoundaryConditions::BoundaryCondition > BnsInitialData ::BoundaryConditions::StarSurface::get_clone ( ) const

inlineoverridevirtual

constexpr Options::String BnsInitialData ::BoundaryConditions::StarSurface::help

staticconstexpr

Initial value:

=

"StarSurface boundary conditions n_i F^i = C/square(alpha) B^i n_i ."

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