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SpECTRE
2021.08.02
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Computes the analytic data for a gauge wave solution described in [7]. More...
#include <GaugeWave.hpp>
Classes | |
| struct | Amplitude |
| struct | Duration |
| struct | ExtractionRadius |
| struct | Frequency |
| struct | Mass |
| struct | PeakTime |
Public Member Functions | |
| WRAPPED_PUPable_decl_template (GaugeWave) | |
| GaugeWave (CkMigrateMessage *msg) noexcept | |
| GaugeWave (double extraction_radius, double mass, double frequency, double amplitude, double peak_time, double duration) noexcept | |
| std::unique_ptr< WorldtubeData > | get_clone () const noexcept override |
| void | pup (PUP::er &p) noexcept override |
Public Member Functions inherited from Cce::Solutions::SphericalMetricData | |
| WRAPPED_PUPable_abstract (SphericalMetricData) | |
| SphericalMetricData (CkMigrateMessage *msg) noexcept | |
| SphericalMetricData (const double extraction_radius) noexcept | |
| void | jacobian (gsl::not_null< SphericaliCartesianJ * > jacobian, size_t l_max) const noexcept |
| void | inverse_jacobian (gsl::not_null< CartesianiSphericalJ * > inverse_jacobian, size_t l_max) const noexcept |
| void | dr_inverse_jacobian (gsl::not_null< CartesianiSphericalJ * > dr_inverse_jacobian, size_t l_max) const noexcept |
| void | pup (PUP::er &p) noexcept override |
Public Member Functions inherited from Cce::Solutions::WorldtubeData | |
| WRAPPED_PUPable_abstract (WorldtubeData) | |
| WorldtubeData (const double extraction_radius) noexcept | |
| WorldtubeData (CkMigrateMessage *msg) noexcept | |
| template<typename... Tags> | |
| tuples::TaggedTuple< Tags... > | variables (const size_t output_l_max, const double time, tmpl::list< Tags... >) const noexcept |
Retrieve worldtube data represented by the analytic solution, at boundary angular resolution l_max and time time More... | |
| void | pup (PUP::er &p) noexcept override |
| virtual std::unique_ptr< Cce::InitializeJ::InitializeJ< false > > | get_initialize_j (const double) const noexcept |
| virtual bool | use_noninertial_news () const noexcept |
Static Public Attributes | |
| static constexpr Options::String | help |
Protected Member Functions | |
| void | prepare_solution (const size_t, const double) const noexcept override |
| A no-op as the gauge wave solution does not have substantial shared computation to prepare before the separate component calculations. More... | |
| void | spherical_metric (gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * > spherical_metric, size_t l_max, double time) const noexcept override |
| Compute the spherical coordinate metric from the closed-form gauge wave metric. More... | |
| void | dr_spherical_metric (gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * > dr_spherical_metric, size_t l_max, double time) const noexcept override |
| Compute the radial derivative of the spherical coordinate metric from the closed-form gauge wave metric. More... | |
| void | dt_spherical_metric (gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * > dt_spherical_metric, size_t l_max, double time) const noexcept override |
| Compute the spherical coordinate metric from the closed-form gauge wave metric. More... | |
| void | variables_impl (gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * > News, size_t l_max, double time, tmpl::type_< Tags::News >) const noexcept override |
| The News vanishes, because the wave is pure gauge. More... | |
| virtual void | variables_impl (gsl::not_null< tnsr::i< DataVector, 3 > * > cartesian_coordinates, size_t output_l_max, double time, tmpl::type_< Tags::CauchyCartesianCoords >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::i< DataVector, 3 > * > dr_cartesian_coordinates, size_t output_l_max, double time, tmpl::type_< Tags::Dr< Tags::CauchyCartesianCoords > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > spacetime_metric, size_t output_l_max, double time, tmpl::type_< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > >) const noexcept=0 |
| Computes the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > dt_spacetime_metric, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept=0 |
| Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > pi, size_t output_l_max, double time, tmpl::type_< GeneralizedHarmonic::Tags::Pi< 3, ::Frame::Inertial > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::iaa< DataVector, 3 > * > d_spacetime_metric, size_t output_l_max, double time, tmpl::type_< GeneralizedHarmonic::Tags::Phi< 3, ::Frame::Inertial > >) const noexcept=0 |
| Computes the spatial derivatives of the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > spatial_metric, size_t output_l_max, double time, tmpl::type_< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > dt_spatial_metric, size_t output_l_max, double time, tmpl::type_< ::Tags::dt< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > dr_spatial_metric, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > shift, size_t output_l_max, double time, tmpl::type_< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > dt_shift, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > dr_shift, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > lapse, size_t output_l_max, double time, tmpl::type_< gr::Tags::Lapse< DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > dt_lapse, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::Lapse< DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > dr_lapse, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::Lapse< DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * > news, size_t output_l_max, double time, tmpl::type_< Tags::News >) const noexcept=0 |
| void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > spacetime_metric, size_t l_max, double time, tmpl::type_< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > >) const noexcept override |
| Computes the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
| void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > dt_spacetime_metric, size_t l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept override |
| Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
| void | variables_impl (gsl::not_null< tnsr::iaa< DataVector, 3 > * > d_spacetime_metric, size_t l_max, double time, tmpl::type_< GeneralizedHarmonic::Tags::Phi< 3, ::Frame::Inertial > >) const noexcept override |
| Computes the spatial derivatives of the Cartesian spacetime metric from the spherical solution provided by the derived classes. More... | |
Protected Member Functions inherited from Cce::Solutions::SphericalMetricData | |
| virtual void | variables_impl (gsl::not_null< tnsr::i< DataVector, 3 > * > cartesian_coordinates, size_t output_l_max, double time, tmpl::type_< Tags::CauchyCartesianCoords >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::i< DataVector, 3 > * > dr_cartesian_coordinates, size_t output_l_max, double time, tmpl::type_< Tags::Dr< Tags::CauchyCartesianCoords > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > spacetime_metric, size_t output_l_max, double time, tmpl::type_< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > >) const noexcept=0 |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > dt_spacetime_metric, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::SpacetimeMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept=0 |
| virtual void | variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > pi, size_t output_l_max, double time, tmpl::type_< GeneralizedHarmonic::Tags::Pi< 3, ::Frame::Inertial > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::iaa< DataVector, 3 > * > d_spacetime_metric, size_t output_l_max, double time, tmpl::type_< GeneralizedHarmonic::Tags::Phi< 3, ::Frame::Inertial > >) const noexcept=0 |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > spatial_metric, size_t output_l_max, double time, tmpl::type_< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > dt_spatial_metric, size_t output_l_max, double time, tmpl::type_< ::Tags::dt< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::ii< DataVector, 3 > * > dr_spatial_metric, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::SpatialMetric< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > shift, size_t output_l_max, double time, tmpl::type_< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > dt_shift, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > dr_shift, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::Shift< 3, ::Frame::Inertial, DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > lapse, size_t output_l_max, double time, tmpl::type_< gr::Tags::Lapse< DataVector > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > dt_lapse, size_t output_l_max, double time, tmpl::type_<::Tags::dt< gr::Tags::Lapse< DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< DataVector > * > dr_lapse, size_t output_l_max, double time, tmpl::type_< Tags::Dr< gr::Tags::Lapse< DataVector > > >) const noexcept |
| virtual void | variables_impl (gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * > news, size_t output_l_max, double time, tmpl::type_< Tags::News >) const noexcept=0 |
Protected Member Functions inherited from Cce::Solutions::WorldtubeData | |
| template<typename Tag > | |
| const auto & | cache_or_compute (const size_t output_l_max, const double time) const noexcept |
Protected Attributes | |
| double | mass_ = std::numeric_limits<double>::signaling_NaN() |
| double | frequency_ = std::numeric_limits<double>::signaling_NaN() |
| double | amplitude_ = std::numeric_limits<double>::signaling_NaN() |
| double | peak_time_ = std::numeric_limits<double>::signaling_NaN() |
| double | duration_ = std::numeric_limits<double>::signaling_NaN() |
Protected Attributes inherited from Cce::Solutions::WorldtubeData | |
| IntermediateCacheTuple | intermediate_cache_ |
| double | extraction_radius_ = std::numeric_limits<double>::quiet_NaN() |
Computes the analytic data for a gauge wave solution described in [7].
This test computes an analytic solution of a pure-gauge perturbation of the Schwarzschild metric. The gauge perturbation is constructed using the time-dependent coordinate transformation of the ingoing Eddington-Finklestein coordinate \(\nu \rightarrow \nu + F(t - r) / r\), where
\[ F(u) = A \sin(\omega u) e^{- (u - u_0)^2 / k^2}. \]
Cce::Solutions::BouncingBlackHole solution.
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overrideprotectedvirtualnoexcept |
Compute the radial derivative of the spherical coordinate metric from the closed-form gauge wave metric.
The transformation of the ingoing Eddington-Finkelstein coordinate produces the radial derivative of the metric components in spherical coordinates:
\begin{align*} \partial_r g_{tt} + \partial_t g_{tt} =& \frac{2}{r^4} \left[r + \partial_u F(u)\right] \left[- M r + (r - 3 M)\partial_u F(u)\right] \\ \partial_r g_{rt} + \partial_t g_{rt} =& - \frac{1}{r^5} \left\{2 M r^3 + 2 r F(u) (r - 3M) + \partial_u F(u)[r^3 + F(u)(3r - 8 M)] + 2 r [\partial_u F(u)]^2 (r - 3M)\right\}\\ \partial_r g_{rr} + \partial_t g_{rr} =& \frac{2}{r^6} \left\{- M r^4 + F(u)^2 (2r - 5M) + \partial_u F(u) r^2 \left[4 M r + \partial_u F(u) (r - 3 M)\right] + F(u) r \left[6 M r + \partial_u F(u) (3r - 8 M)\right]\right\} \\ g_{\theta \theta} =& 2 r \\ g_{\phi \phi} =& 2 r \sin^2(\theta), \end{align*}
and all other components vanish (these formulae are obtained simply by applying radial derivatives to those given in GaugeWave::spherical_metric()). Here, \(F(u)\) is defined as
\begin{align*} F(u) &= A \sin(\omega u) e^{-(u - u_0)^2 /k^2},\\ \partial_u F(u) &= A \left[-2 \frac{u - u_0}{k^2} \sin(\omega u) + \omega \cos(\omega u)\right] e^{-(u - u_0)^2 / k^2}. \end{align*}
Implements Cce::Solutions::SphericalMetricData.
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overrideprotectedvirtualnoexcept |
Compute the spherical coordinate metric from the closed-form gauge wave metric.
The transformation of the ingoing Eddington-Finkelstein coordinate produces metric components in spherical coordinates:
\begin{align*} \partial_t g_{tt} =& \frac{-2 \partial_u^2 F(u)}{r^3} \left(r - 2 M\right) \left(r + \partial_u F(u)\right) \\ \partial_t g_{rt} =& \frac{1}{r^4} \Bigg\{\partial_u^2 F(u) \left[2 M r^2 + \left(r - 2 M\right) (r \partial_u F(u) + F(u))\right] \\ &+ \left[r + \partial_u F(u)\right] \left(r - 2M\right) \left[r \partial_u^2 F(u) + \partial_u F(u) \right]\Bigg\} \\ \partial_t g_{rr} =& \frac{1}{r^5}\Bigg\{-\left[r \partial_u^2 F(u) + \partial_u F(u)\right] \left[r^3 + 2 M r^2 + \left(r - 2 M\right) \left(r \partial_u F(u) + F(u)\right)\right]\\ &+ \left[r^2 - r \partial_u F(u) - F(u)\right] \left(r - 2 M\right) \left[r \partial_u^2 F(u) + \partial_u F(u)\right]\Bigg\} \\ \partial_t g_{\theta \theta} =& 0 \\ \partial_t g_{\phi \phi} =& 0, \end{align*}
and all other components vanish. Here, \(F(u)\) is defined as
\begin{align*} F(u) &= A \sin(\omega u) e^{-(u - u_0)^2 /k^2},\\ \partial_u F(u) &= A \left[-2 \frac{u - u_0}{k^2} \sin(\omega u) + \omega \cos(\omega u)\right] e^{-(u - u_0)^2 / k^2},\\ \partial^2_u F(u) &= \frac{A}{k^4} \left\{-4 k^2 \omega (u - u_0) \cos(\omega u) + \left[-2 k^2 + 4 (u - u_0)^2 - k^4 \omega^2\right] \sin(\omega u)\right\} e^{-(u - u_0) / k^2} \end{align*}
Implements Cce::Solutions::SphericalMetricData.
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overridevirtualnoexcept |
Implements Cce::Solutions::WorldtubeData.
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inlineoverrideprotectedvirtualnoexcept |
A no-op as the gauge wave solution does not have substantial shared computation to prepare before the separate component calculations.
Implements Cce::Solutions::WorldtubeData.
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overrideprotectedvirtualnoexcept |
Compute the spherical coordinate metric from the closed-form gauge wave metric.
The transformation of the ingoing Eddington-Finkelstein coordinate produces metric components in spherical coordinates (identical up to minor manipulations of the metric given in Eq. (149) of [7]):
\begin{align*} g_{tt} &= \frac{-1}{r^3}\left(r - 2 M\right) \left[r + \partial_u F(u)\right]^2\\ g_{rt} &= \frac{1}{r^4} \left[r + \partial_u F(u)\right] \left\{2 M r^2 + \left(r - 2 M\right) \left[r \partial_u F(u) + F(u)\right]\right\} \\ g_{rr} &= \frac{1}{r^5} \left[r^2 - r \partial_u F(u) - F(u)\right] \left\{r^3 + 2 M r^2 + \left(r - 2 M\right) \left[r \partial_u F(u) + F(u)\right]\right\} \\ g_{\theta \theta} &= r^2 \\ g_{\phi \phi} &= r^2 \sin^2(\theta), \end{align*}
and all other components vanish. Here, \(F(u)\) is defined as
\begin{align*} F(u) &= A \sin(\omega u) e^{-(u - u_0)^2 /k^2},\\ \partial_u F(u) &= A \left[-2 \frac{u - u_0}{k^2} \sin(\omega u) + \omega \cos(\omega u)\right] e^{-(u - u_0)^2 / k^2}. \end{align*}
Implements Cce::Solutions::SphericalMetricData.
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Reimplemented from Cce::Solutions::WorldtubeData.
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Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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overrideprotectedvirtualnoexcept |
The News vanishes, because the wave is pure gauge.
Implements Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Implements Cce::Solutions::WorldtubeData.
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overrideprotectedvirtualnoexcept |
Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide the time derivative of the spherical metric data via the virtual function SphericalMetricData::dt_spherical_metric() at a resolution determined by the l_max argument. This function performs the coordinate transformation using the Jacobian computed from SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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protectedvirtualnoexcept |
Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide the time derivative of the spherical metric data via the virtual function SphericalMetricData::dt_spherical_metric() at a resolution determined by the l_max argument. This function performs the coordinate transformation using the Jacobian computed from SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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overrideprotectedvirtualnoexcept |
Computes the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide spherical metric data via the virtual function SphericalMetricData::spherical_metric() at a resolution determined by the l_max argument. This function performs the coordinate transformation using the Jacobian computed from SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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protectedvirtualnoexcept |
Computes the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide spherical metric data via the virtual function SphericalMetricData::spherical_metric() at a resolution determined by the l_max argument. This function performs the coordinate transformation using the Jacobian computed from SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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overrideprotectedvirtualnoexcept |
Computes the spatial derivatives of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide the radial derivative of the spherical metric data via the virtual function SphericalMetricData::dr_spherical_metric() at a resolution determined by the l_max_ argument. This function performs the additional angular derivatives necessary to assemble the full spatial derivative and performs the coordinate transformation to Cartesian coordinates via the Jacobians computed in SphericalMetricData::inverse_jacobian() and SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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protectedvirtualnoexcept |
Computes the spatial derivatives of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
The derived classes provide the radial derivative of the spherical metric data via the virtual function SphericalMetricData::dr_spherical_metric() at a resolution determined by the l_max_ argument. This function performs the additional angular derivatives necessary to assemble the full spatial derivative and performs the coordinate transformation to Cartesian coordinates via the Jacobians computed in SphericalMetricData::inverse_jacobian() and SphericalMetricData::inverse_jacobian().
Reimplemented from Cce::Solutions::SphericalMetricData.
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Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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protectedvirtualnoexcept |
Reimplemented from Cce::Solutions::WorldtubeData.
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staticconstexpr |