Dispatcher to compute the puncture/singular field for a scalar charge on a generic orbit in Schwarzschild or Kerr spacetime. The Kerr puncture reduces to Schwarzsschild for zero spin but is faster to evaluate.
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#include <PunctureField.hpp>
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| enum class | Type { Schwarzschild
, Kerr
} |
| using | options |
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| PunctureField (const Schwarzschild &schwarzschild, const Options::Context &context={}) |
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| PunctureField (const Kerr &kerr, const Options::Context &context={}) |
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void | pup (PUP::er &p) |
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Type | type () const |
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size_t | expansion_order () const |
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double | black_hole_mass () const |
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double | spin_along_z_axis () const |
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void | apply_puncture (gsl::not_null< Variables< tmpl::list< CurvedScalarWave::Tags::Psi, ::Tags::dt< CurvedScalarWave::Tags::Psi >, ::Tags::deriv< CurvedScalarWave::Tags::Psi, tmpl::size_t< 3 >, Frame::Inertial > > > * > result, const tnsr::I< DataVector, 3, Frame::Inertial > ¢ered_coords, const tnsr::I< double, 3 > &particle_position, const tnsr::I< double, 3 > &particle_velocity, const tnsr::I< double, 3 > &particle_acceleration) const |
| | Compute and write the puncture field and its derivatives for the configured puncture model and expansion order.
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void | apply_acceleration_terms (gsl::not_null< Variables< tmpl::list< CurvedScalarWave::Tags::Psi, ::Tags::dt< CurvedScalarWave::Tags::Psi >, ::Tags::deriv< CurvedScalarWave::Tags::Psi, tmpl::size_t< 3 >, Frame::Inertial > > > * > result, const tnsr::I< DataVector, 3, Frame::Inertial > ¢ered_coords, const tnsr::I< double, 3 > &particle_position, const tnsr::I< double, 3 > &particle_velocity, const tnsr::I< double, 3 > &particle_acceleration, double ft, double fx, double fy, double dt_ft, double dt_fx, double dt_fy, double Du_ft, double Du_fx, double Du_fy, double dt_Du_ft, double dt_Du_fx, double dt_Du_fy) const |
| | Compute and write the corrections to the puncture field for the configured puncture model and expansion order. These terms arise at non-geodesic accelerations such as the self-force.
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Dispatcher to compute the puncture/singular field for a scalar charge on a generic orbit in Schwarzschild or Kerr spacetime. The Kerr puncture reduces to Schwarzsschild for zero spin but is faster to evaluate.
◆ options
| using CurvedScalarWave::Worldtube::PunctureField::options |
Initial value: tmpl::list<
Provide multiple ways to construct a class.
Definition Options.hpp:93
◆ help
Initial value:= {
"Configuration and dispatcher for puncture-field expressions. Choose "
"either Schwarzschild or Kerr."}
The documentation for this class was generated from the following file:
- src/Evolution/Systems/CurvedScalarWave/Worldtube/PunctureField.hpp