An analytic solution representing a specialization of the radiative Robinson-Trautman solution described in [59]. More...

#include <RobinsonTrautman.hpp>

Classes
struct	ExtractionRadius
struct	InitialModes
struct	LMax
struct	StartTime
struct	Tolerance

Public Types
using	options
Public Types inherited from Cce::Solutions::WorldtubeData
using	creatable_classes
using	tags
	The set of available tags provided by the analytic solution.

Public Member Functions
	WRAPPED_PUPable_decl_template (RobinsonTrautman)
	RobinsonTrautman (CkMigrateMessage *msg)
	RobinsonTrautman (std::vector< std::complex< double > > initial_modes, double extraction_radius, size_t l_max, double tolerance, double start_time, const Options::Context &context)
std::unique_ptr< WorldtubeData >	get_clone () const override
void	pup (PUP::er &p) override
bool	use_noninertial_news () const override
Public Member Functions inherited from Cce::Solutions::SphericalMetricData
	WRAPPED_PUPable_abstract (SphericalMetricData)
	SphericalMetricData (CkMigrateMessage *msg)
	SphericalMetricData (const double extraction_radius)
void	jacobian (gsl::not_null< SphericaliCartesianJ * > jacobian, size_t l_max) const
void	inverse_jacobian (gsl::not_null< CartesianiSphericalJ * > inverse_jacobian, size_t l_max) const
void	dr_inverse_jacobian (gsl::not_null< CartesianiSphericalJ * > dr_inverse_jacobian, size_t l_max) const
void	pup (PUP::er &p) override
Public Member Functions inherited from Cce::Solutions::WorldtubeData
	WRAPPED_PUPable_abstract (WorldtubeData)
	WorldtubeData (const double extraction_radius)
	WorldtubeData (CkMigrateMessage *msg)
template<typename... Tags>
tuples::TaggedTuple< Tags... >	variables (const size_t output_l_max, const double time, tmpl::list< Tags... >) const
	Retrieve worldtube data represented by the analytic solution, at boundary angular resolution l_max and time time
void	pup (PUP::er &p) override
virtual std::unique_ptr< Cce::InitializeJ::InitializeJ< false > >	get_initialize_j (const double) const

Static Public Attributes
static constexpr Options::String	help

Protected Member Functions
void	prepare_solution (size_t output_l_max, double time) const override
	The Robinson-Trautman solution performs the time-stepping to advance the internal member scalar used to generate the metric solution to the correct state for time.
void	spherical_metric (gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * > spherical_metric, size_t l_max, double time) const override
	Compute the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).
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 override
	Compute radial derivative of the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).
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 override
	Compute time derivative of the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).
void	variables_impl (gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * > News, size_t l_max, double time, tmpl::type_< Tags::News >) const override
	Compute the news associated with the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).
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
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
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< DataVector, 3 > >) const=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< DataVector, 3 > > >) const=0
virtual void	variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > pi, size_t output_l_max, double time, tmpl::type_< gh::Tags::Pi< DataVector, 3 > >) const
virtual void	variables_impl (gsl::not_null< tnsr::iaa< DataVector, 3 > * > d_spacetime_metric, size_t output_l_max, double time, tmpl::type_< gh::Tags::Phi< DataVector, 3 > >) const=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< DataVector, 3 > >) const
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< DataVector, 3 > > >) const
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< DataVector, 3 > > >) const
virtual void	variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > shift, size_t output_l_max, double time, tmpl::type_< gr::Tags::Shift< DataVector, 3 > >) const
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< DataVector, 3 > > >) const
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< DataVector, 3 > > >) const
virtual void	variables_impl (gsl::not_null< Scalar< DataVector > * > lapse, size_t output_l_max, double time, tmpl::type_< gr::Tags::Lapse< DataVector > >) const
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
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
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< DataVector, 3 > > >) const override
	Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
Protected Member Functions inherited from Cce::Solutions::SphericalMetricData
void	variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > spacetime_metric, size_t l_max, double time, tmpl::type_< gr::Tags::SpacetimeMetric< DataVector, 3 > >) const override
	Computes the Cartesian spacetime metric from the spherical solution provided by the derived classes.
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< DataVector, 3 > > >) const override
	Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
void	variables_impl (gsl::not_null< tnsr::iaa< DataVector, 3 > * > d_spacetime_metric, size_t l_max, double time, tmpl::type_< gh::Tags::Phi< DataVector, 3 > >) const override
	Computes the spatial derivatives of the Cartesian spacetime metric from the spherical solution provided by the derived classes.
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
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
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< DataVector, 3 > > >) const=0
virtual void	variables_impl (gsl::not_null< tnsr::aa< DataVector, 3 > * > pi, size_t output_l_max, double time, tmpl::type_< gh::Tags::Pi< DataVector, 3 > >) const
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< DataVector, 3 > >) const
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< DataVector, 3 > > >) const
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< DataVector, 3 > > >) const
virtual void	variables_impl (gsl::not_null< tnsr::I< DataVector, 3 > * > shift, size_t output_l_max, double time, tmpl::type_< gr::Tags::Shift< DataVector, 3 > >) const
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< DataVector, 3 > > >) const
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< DataVector, 3 > > >) const
virtual void	variables_impl (gsl::not_null< Scalar< DataVector > * > lapse, size_t output_l_max, double time, tmpl::type_< gr::Tags::Lapse< DataVector > >) const
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
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
virtual void	variables_impl (gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * > news, size_t output_l_max, double time, tmpl::type_< Tags::News >) const=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

Additional Inherited Members
Static Public Member Functions inherited from Cce::Solutions::SphericalMetricData
static void	dr_jacobian (gsl::not_null< SphericaliCartesianJ * > dr_jacobian, size_t l_max)
Protected Types inherited from Cce::Solutions::WorldtubeData
using	IntermediateCacheTuple
Protected Attributes inherited from Cce::Solutions::WorldtubeData
IntermediateCacheTuple	intermediate_cache_
double	extraction_radius_ = std::numeric_limits<double>::quiet_NaN()

Detailed Description

An analytic solution representing a specialization of the radiative Robinson-Trautman solution described in [59].

Details

This solution is not quite analytic, in the sense that there is a single scalar field that must be evolved. Ultimately, it is a partial specialization of the Characteristic equations such that \(J = 0\) and the evolution equations have been manipulated to give a time evolution equation for \(e^{-2 \beta}\), which is equivalent to the Robinson-Trautman scalar \(\omega_{\text{RT}}\) (denoted \(W\) in [59] – we deviate from their notation because the symbol \(W\) is already used elsewhere in the CCE system).

Note: The value of \(\omega_{\text{RT}}\) should be real and near 1, which is imposed by the solution itself, any modes specified in the input file are treated as perturbations to the leading value of 1.0 for the Robinson-Trautman scalar \(\omega_{\text{RT}}\).; The use of substep time-steppers in conjunction with RobinsonTrautman analytic data is explictly forbidden by checks in Cce::Actions::InitializeWorldtubeBoundary. The reason is that any time the RobinsonTrautman receives a request for data at a time in the past of its current state, it must re-start its internal time stepper from the beginning of the evolution. This is a reasonable cost for multistep methods that only have non-ordered time steps during self-start, but will lead to \(\mathcal O(N^2)\) internal steps in the RobinsonTrautman solution if a substep method is used, where \(N\) is the number of steps performed by the substep method. If you find an unavoidable need to use RobinsonTrautman with a substep method, you will either need to only do so for very short evolutions, or need to write more sophisticated caching of the internal time step data.

Member Typedef Documentation

◆ options

using Cce::Solutions::RobinsonTrautman::options

Initial value:

tmpl::list<InitialModes, ExtractionRadius, LMax, Tolerance, StartTime>

Member Function Documentation

◆ dr_spherical_metric()

void Cce::Solutions::RobinsonTrautman::dr_spherical_metric	(	gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * >	dr_spherical_metric,
		size_t	l_max,
		double	time ) const

overrideprotectedvirtual

Compute radial derivative of the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).

Details

The radial derivative (at constant time t) of the Robinson-Trautman solution is obtained by differentiating the expressions from the documentation for RobinsonTrautman::spherical_metric():

\begin{align*}(\partial_r g_{a b} + \partial_t g_{a b}) dx^a dx^b = - (\omega_{\text{RT}} (r \partial_r W + W) - 2 r U \bar U - r^2 (\bar U\partial_r U + U \partial_r \bar U)) (dt - dr)^2 - 2 r U^A q_{A B} dx^B (dt - dr) + 2 r q_{A B} dx^A dx^B \end{align*}

where \(q_{A B}\) represents the angular unit sphere metric, and the remaining Bondi-Sachs scalars and angular tensors are defined in terms of the Robinson-Trautman scalar \(\omega_{\text{RT}}\)

\begin{align*}W &= \frac{1}{r}\left(\omega_{\text{RT}} + \eth \bar \eth \omega_{\text{RT}} - 1\right) - \frac{2}{r^2 \omega_{\text{RT}}^2}\\ \partial_r W &= -\frac{1}{r^2} \left(\omega_{\text{RT}} + \eth \bar \eth \omega_{\text{RT}} - 1\right) + \frac{4}{r^3 \omega_{\text{RT}}^2}\\ U &\equiv U^A q_A = \frac{\eth \omega_{\text{RT}}}{r}. \end{align*}

and \(q_A\) is the angular dyad on the unit sphere. The Robinson-Trautman scalar \(\omega_{\text{RT}}\) is independent of the Bondi radius \(r\), so all radial derivatives of \(\omega_{\text{RT}}\) have been dropped

Implements Cce::Solutions::SphericalMetricData.

◆ dt_spherical_metric()

void Cce::Solutions::RobinsonTrautman::dt_spherical_metric	(	gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * >	dt_spherical_metric,
		size_t	l_max,
		double	time ) const

overrideprotectedvirtual

Compute time derivative of the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).

Details

The time derivative of the Robinson-Trautman solution is obtained by differentiating the expressions from the documentation for RobinsonTrautman::spherical_metric():

\begin{align*}\partial_t g_{a b} dx^a dx^b = -( \partial_u \omega_{\text{RT}} (r W + 1) + \omega_{\text{RT}} \partial_u W - r^2 (\bar U \partial_u U + U \partial_u \bar U)) (dt - dr)^2 - 2 \partial_u \omega_{\text{RT}} (dt - dr) dr - 2 r^2 \partial_u U^A q_{AB} dx^B (dt - dr), \end{align*}

where \(q_{A B}\) represents the angular unit sphere metric, and the remaining Bondi-Sachs scalars and angular tensors are defined in terms of the Robinson-Trautman scalar \(\omega_{\text{RT}}\)

\begin{align*}W &= \frac{1}{r}\left(\omega_{\text{RT}} + \eth \bar \eth \omega_{\text{RT}} - 1\right) - \frac{2}{r^2 \omega_{\text{RT}}^2}\\ \partial_u W &= \frac{1}{r}\left(\partial_u \omega_{\text{RT}} + \eth \bar \eth \partial_u \omega_{\text{RT}}\right) + \frac{4 \partial_u \omega_{\text{RT}}}{r^2 \omega_{\text{RT}}^3} \\ \partial_u U &= q_A \partial_u U^A = \frac{\eth \partial_u \omega_{\text{RT}}}{r}, \end{align*}

and \(q_A\) is the angular dyad on the unit sphere; and the time derivative of the Robinson-Trautman scalar \(\omega_{\text{RT}}\) is

\[\partial_u \omega_{\text{RT}} = \frac{1}{12} \left(-\omega^4_{\text{RT}} \eth^2 \bar \eth^2 \omega_{\text{RT}} + \omega_{\text{RT}}^3 (\eth^2 \omega_{\text{RT}}) (\bar \eth^2 \omega_{\text{RT}}) \right) \]

Implements Cce::Solutions::SphericalMetricData.

◆ get_clone()

std::unique_ptr< WorldtubeData > Cce::Solutions::RobinsonTrautman::get_clone ( ) const

overridevirtual

Implements Cce::Solutions::WorldtubeData.

◆ prepare_solution()

void Cce::Solutions::RobinsonTrautman::prepare_solution	(	size_t	output_l_max,
		double	time ) const

overrideprotectedvirtual

The Robinson-Trautman solution performs the time-stepping to advance the internal member scalar used to generate the metric solution to the correct state for time.

Details

The generating scalar \(\omega_{\text{RT}}\) is evolved using equation (2.5) from [59] (manipulated to a form convenient for our numerical utilities)

\[\partial_u \omega_{\text{RT}} = - \left(\omega^4_{\text{RT}} \eth^2 \bar \eth^2 \omega_{\text{RT}} - \omega_{\text{RT}}^3 (\eth^2 \omega_{\text{RT}}) (\bar \eth^2 \omega_{\text{RT}}) \right) \]

As the scalar \(\omega_{\text{RT}}\) is evolved, it is filtered by zeroing the highest two angular modes.

Implements Cce::Solutions::WorldtubeData.

◆ spherical_metric()

void Cce::Solutions::RobinsonTrautman::spherical_metric	(	gsl::not_null< tnsr::aa< DataVector, 3, ::Frame::Spherical<::Frame::Inertial > > * >	spherical_metric,
		size_t	l_max,
		double	time ) const

overrideprotectedvirtual

Compute the spherical coordinate metric of the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).

Details

The spacetime metric of the Robinson-Trautman solution can be expressed as a specialization of the Bondi-Sachs metric (note the metric signature change as compared to equation (1.2) from [59])

\[ds^2 = -((r W + 1) \omega_{\text{RT}} - r^2 U \bar U) (dt - dr)^2 - 2 \omega_{\text{RT}} (dt - dr) dr - 2 r^2 U^A q_{AB} dx^B (dt - dr) + r^2 q_{A B} dx^A dx^B, \]

where \(q_{A B}\) represents the angular unit sphere metric, and the remaining Bondi-Sachs scalars and angular tensors are defined in terms of the Robinson-Trautman scalar \(\omega_{\text{RT}}\)

\begin{align*}W &= \frac{1}{r}\left(\omega_{\text{RT}} + \eth \bar \eth \omega_{\text{RT}} - 1\right) - \frac{2}{r^2 \omega_{\text{RT}}^2}\\ U &\equiv U^A q_A = \frac{\eth \omega_{\text{RT}}}{r}. \end{align*}

and \(q_A\) is the angular dyad on the unit sphere.

The angular part of the metric can be expressed in terms of the \(U\) scalar as

\begin{align*}g_{u \theta} &= r^2 \Re U\\ g_{u \phi} &= r^2 \Im U \end{align*}

Implements Cce::Solutions::SphericalMetricData.

◆ use_noninertial_news()

bool Cce::Solutions::RobinsonTrautman::use_noninertial_news ( ) const

inlineoverridevirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [1/17]

virtual void Cce::Solutions::WorldtubeData::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

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [2/17]

virtual void Cce::Solutions::WorldtubeData::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

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [3/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< Scalar< DataVector > * >	lapse,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gr::Tags::Lapse< DataVector > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [4/17]

void Cce::Solutions::RobinsonTrautman::variables_impl	(	gsl::not_null< Scalar< SpinWeighted< ComplexDataVector, -2 > > * >	News,
		size_t	l_max,
		double	time,
		tmpl::type_< Tags::News >	) const

overrideprotectedvirtual

Compute the news associated with the Robinson-Trautman solution generated by the time-evolved scalar \(\omega_{\text{RT}}\).

Details

The Bondi-Sachs news in the Robinson-Trautman solution is

\begin{align*}N = \frac{\bar \eth \bar \eth \omega_{\text{RT}}}{\omega_{\text{RT}}} \end{align*}

Implements Cce::Solutions::WorldtubeData.

◆ variables_impl() [5/17]

void Cce::Solutions::SphericalMetricData::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< DataVector, 3 > > >	) const

overrideprotected

Computes the time derivative of the Cartesian spacetime metric from the spherical solution provided by the derived classes.

Details

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().

◆ variables_impl() [6/17]

virtual void Cce::Solutions::WorldtubeData::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< DataVector, 3 > > >	) const

protectedvirtual

Implements Cce::Solutions::WorldtubeData.

◆ variables_impl() [7/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::aa< DataVector, 3 > * >	pi,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gh::Tags::Pi< DataVector, 3 > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [8/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::aa< DataVector, 3 > * >	spacetime_metric,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gr::Tags::SpacetimeMetric< DataVector, 3 > >	) const

protectedvirtual

Implements Cce::Solutions::WorldtubeData.

◆ variables_impl() [9/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::i< DataVector, 3 > * >	cartesian_coordinates,
		size_t	output_l_max,
		double	time,
		tmpl::type_< Tags::CauchyCartesianCoords >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [10/17]

virtual void Cce::Solutions::WorldtubeData::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

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [11/17]

virtual void Cce::Solutions::WorldtubeData::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< DataVector, 3 > > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [12/17]

virtual void Cce::Solutions::WorldtubeData::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< DataVector, 3 > > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [13/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::I< DataVector, 3 > * >	shift,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gr::Tags::Shift< DataVector, 3 > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [14/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::iaa< DataVector, 3 > * >	d_spacetime_metric,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gh::Tags::Phi< DataVector, 3 > >	) const

protectedvirtual

Implements Cce::Solutions::WorldtubeData.

◆ variables_impl() [15/17]

virtual void Cce::Solutions::WorldtubeData::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< DataVector, 3 > > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [16/17]

virtual void Cce::Solutions::WorldtubeData::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< DataVector, 3 > > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

◆ variables_impl() [17/17]

virtual void Cce::Solutions::WorldtubeData::variables_impl	(	gsl::not_null< tnsr::ii< DataVector, 3 > * >	spatial_metric,
		size_t	output_l_max,
		double	time,
		tmpl::type_< gr::Tags::SpatialMetric< DataVector, 3 > >	) const

protectedvirtual

Reimplemented from Cce::Solutions::WorldtubeData.

Member Data Documentation

◆ help

Options::String Cce::Solutions::RobinsonTrautman::help

staticconstexpr

Initial value:

= {
      "Analytic solution representing worldtube data for the nonlinear "
      "semi-analytic Robinson-Trautman metric, which requires a single "
      "scalar on the boundary to be evolved to determine the metric"}

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

src/Evolution/Systems/Cce/AnalyticSolutions/RobinsonTrautman.hpp

Classes

Public Types

Public Member Functions

Static Public Attributes

Protected Member Functions

Additional Inherited Members

Detailed Description

Details

Member Typedef Documentation

◆ options

Member Function Documentation

◆ dr_spherical_metric()

Details

◆ dt_spherical_metric()

Details

◆ get_clone()

◆ prepare_solution()

Details

◆ spherical_metric()

Details

◆ use_noninertial_news()

◆ variables_impl() [1/17]

◆ variables_impl() [2/17]

◆ variables_impl() [3/17]

◆ variables_impl() [4/17]

Details

◆ variables_impl() [5/17]

Details

◆ variables_impl() [6/17]

◆ variables_impl() [7/17]

◆ variables_impl() [8/17]

◆ variables_impl() [9/17]

◆ variables_impl() [10/17]

◆ variables_impl() [11/17]

◆ variables_impl() [12/17]

◆ variables_impl() [13/17]

◆ variables_impl() [14/17]

◆ variables_impl() [15/17]

◆ variables_impl() [16/17]

◆ variables_impl() [17/17]

Member Data Documentation

◆ help