SpECTRE  v2024.05.11
gh::BoundaryConditions::ConstraintPreservingBjorhus< Dim > Class Template Referencefinal

Sets constraint preserving boundary conditions using the Bjorhus method. More...

#include <Bjorhus.hpp>

Classes

struct  TypeOptionTag
 

Public Types

using options = tmpl::list< TypeOptionTag >
 
using dg_interior_evolved_variables_tags = tmpl::list< gr::Tags::SpacetimeMetric< DataVector, Dim >, Tags::Pi< DataVector, Dim >, Tags::Phi< DataVector, Dim > >
 
using dg_interior_temporary_tags = tmpl::list< domain::Tags::Coordinates< Dim, Frame::Inertial >, ConstraintDamping::Tags::ConstraintGamma1, ConstraintDamping::Tags::ConstraintGamma2, gr::Tags::Lapse< DataVector >, gr::Tags::Shift< DataVector, Dim >, gr::Tags::InverseSpacetimeMetric< DataVector, Dim >, gr::Tags::SpacetimeNormalVector< DataVector, Dim >, Tags::ThreeIndexConstraint< DataVector, Dim >, Tags::GaugeH< DataVector, Dim >, Tags::SpacetimeDerivGaugeH< DataVector, Dim > >
 
using dg_interior_dt_vars_tags = tmpl::list<::Tags::dt< gr::Tags::SpacetimeMetric< DataVector, Dim > >, ::Tags::dt< Tags::Pi< DataVector, Dim > >, ::Tags::dt< Tags::Phi< DataVector, Dim > > >
 
using dg_interior_deriv_vars_tags = tmpl::list<::Tags::deriv< gr::Tags::SpacetimeMetric< DataVector, Dim >, tmpl::size_t< Dim >, Frame::Inertial >, ::Tags::deriv< Tags::Pi< DataVector, Dim >, tmpl::size_t< Dim >, Frame::Inertial >, ::Tags::deriv< Tags::Phi< DataVector, Dim >, tmpl::size_t< Dim >, Frame::Inertial > >
 
using dg_gridless_tags = tmpl::list<>
 

Public Member Functions

 ConstraintPreservingBjorhus (detail::ConstraintPreservingBjorhusType type)
 
 ConstraintPreservingBjorhus (CkMigrateMessage *msg)
 
 WRAPPED_PUPable_decl_base_template (domain::BoundaryConditions::BoundaryCondition, ConstraintPreservingBjorhus)
 
auto get_clone () const -> std::unique_ptr< domain::BoundaryConditions::BoundaryCondition > override
 
void pup (PUP::er &p) override
 
std::optional< std::stringdg_time_derivative (gsl::not_null< tnsr::aa< DataVector, Dim, Frame::Inertial > * > dt_spacetime_metric_correction, gsl::not_null< tnsr::aa< DataVector, Dim, Frame::Inertial > * > dt_pi_correction, gsl::not_null< tnsr::iaa< DataVector, Dim, Frame::Inertial > * > dt_phi_correction, const std::optional< tnsr::I< DataVector, Dim, Frame::Inertial > > &face_mesh_velocity, const tnsr::i< DataVector, Dim, Frame::Inertial > &normal_covector, const tnsr::I< DataVector, Dim, Frame::Inertial > &, const tnsr::aa< DataVector, Dim, Frame::Inertial > &spacetime_metric, const tnsr::aa< DataVector, Dim, Frame::Inertial > &pi, const tnsr::iaa< DataVector, Dim, Frame::Inertial > &phi, const tnsr::I< DataVector, Dim, Frame::Inertial > &coords, const Scalar< DataVector > &gamma1, const Scalar< DataVector > &gamma2, const Scalar< DataVector > &lapse, const tnsr::I< DataVector, Dim, Frame::Inertial > &shift, const tnsr::AA< DataVector, Dim, Frame::Inertial > &inverse_spacetime_metric, const tnsr::A< DataVector, Dim, Frame::Inertial > &spacetime_unit_normal_vector, const tnsr::iaa< DataVector, Dim, Frame::Inertial > &three_index_constraint, const tnsr::a< DataVector, Dim, Frame::Inertial > &gauge_source, const tnsr::ab< DataVector, Dim, Frame::Inertial > &spacetime_deriv_gauge_source, const tnsr::aa< DataVector, Dim, Frame::Inertial > &logical_dt_spacetime_metric, const tnsr::aa< DataVector, Dim, Frame::Inertial > &logical_dt_pi, const tnsr::iaa< DataVector, Dim, Frame::Inertial > &logical_dt_phi, const tnsr::iaa< DataVector, Dim, Frame::Inertial > &d_spacetime_metric, const tnsr::iaa< DataVector, Dim, Frame::Inertial > &d_pi, const tnsr::ijaa< DataVector, Dim, Frame::Inertial > &d_phi) const
 
- Public Member Functions inherited from gh::BoundaryConditions::BoundaryCondition< Dim >
 BoundaryCondition (BoundaryCondition &&)=default
 
BoundaryConditionoperator= (BoundaryCondition &&)=default
 
 BoundaryCondition (const BoundaryCondition &)=default
 
BoundaryConditionoperator= (const BoundaryCondition &)=default
 
 BoundaryCondition (CkMigrateMessage *msg)
 
void pup (PUP::er &p) override
 
- Public Member Functions inherited from domain::BoundaryConditions::BoundaryCondition
 BoundaryCondition (BoundaryCondition &&)=default
 
BoundaryConditionoperator= (BoundaryCondition &&)=default
 
 BoundaryCondition (const BoundaryCondition &)=default
 
BoundaryConditionoperator= (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 std::string name ()
 

Static Public Attributes

static constexpr Options::String help
 
static constexpr evolution::BoundaryConditions::Type bc_type
 

Detailed Description

template<size_t Dim>
class gh::BoundaryConditions::ConstraintPreservingBjorhus< Dim >

Sets constraint preserving boundary conditions using the Bjorhus method.

Details

Boundary conditions for the generalized harmonic evolution system can be divided in to three parts, constraint-preserving, physical and gauge boundary conditions.

The generalized harmonic (GH) evolution system is a first-order reduction of Einstein equations brought about by the imposition of GH gauge. This introduces constraints on the free (evolved) variables in addition to the standard Hamiltonian and momentum constraints. The constraint-preserving portion of the boundary conditions is designed to prevent the influx of constraint violations from external faces of the evolution domain, by damping them away on a controlled and short time-scale. These conditions are imposed as corrections to the characteristic projections of the right-hand-sides of the GH evolution equations (i.e. using Bjorhus' method [22]), as written down in Eq. (63) - (65) of [118] . In addition to these equations, the fourth projection is simply frozen in the unlikely case its coordinate speed becomes negative, i.e. \(d_t u^{\hat{1}+}{}_{ab}=0\) (in the notation of [118]). The gauge degrees of freedom are controlled by imposing a Sommerfeld-type condition ( \(L=0\) member of the hierarchy derived in [16]) that allow gauge perturbations to pass through the boundary without strong reflections. These assume a spherical outer boundary, and can be written down as in Eq. (25) of [159] . Finally, the physical boundary conditions control the influx of inward propagating gravitational-wave solutions from the external boundaries. These are derived by considering the evolution system of the Weyl curvature tensor, and controlling the inward propagating characteristics of the system that are proportional to the Newman-Penrose curvature spinor components \(\Psi_4\) and \(\Psi_0\). Here we use Eq. (68) of [118] to disallow any incoming waves. It is to be noted that all the above conditions are also imposed on characteristic modes with speeds exactly zero.

This class provides two choices of combinations of the above corrections:

  • ConstraintPreserving : this imposes the constraint-preserving and gauge-controlling corrections;
  • ConstraintPreservingPhysical : this additionally restricts the influx of any physical gravitational waves from the outer boundary, in addition to preventing the influx of constraint violations and gauge perturbations.

We refer to Bjorhus::constraint_preserving_bjorhus_corrections_dt_v_psi(), Bjorhus::constraint_preserving_bjorhus_corrections_dt_v_zero(), Bjorhus::constraint_preserving_bjorhus_corrections_dt_v_minus(), and Bjorhus::constraint_preserving_physical_bjorhus_corrections_dt_v_minus() for the further details on implementation.

Note
These boundary conditions assume a spherical outer boundary. Also, we do not yet have an option to inject incoming gravitational waves at the outer boundary.

Member Function Documentation

◆ get_clone()

Member Data Documentation

◆ bc_type

template<size_t Dim>
constexpr evolution::BoundaryConditions::Type gh::BoundaryConditions::ConstraintPreservingBjorhus< Dim >::bc_type
staticconstexpr
Initial value:
=
evolution::BoundaryConditions::Type::TimeDerivative

◆ help

template<size_t Dim>
constexpr Options::String gh::BoundaryConditions::ConstraintPreservingBjorhus< Dim >::help
staticconstexpr
Initial value:
{
"ConstraintPreservingBjorhus boundary conditions setting the value of the"
"time derivatives of the spacetime metric, Phi and Pi to expressions that"
"prevent the influx of constraint violations and reflections."}

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